radlw_main.F90

 
 
!!!!!  ==============================================================  !!!!!
!!!!!               lw-rrtm3 radiation package description             !!!!!
!!!!!  ==============================================================  !!!!!
!                                                                          !
!   this package includes ncep's modifications of the rrtmg-lw radiation   !
!   code from aer inc.                                                     !
!                                                                          !
!    the lw-rrtm3 package includes these parts:                            !
!                                                                          !
!       'radlw_rrtm3_param.f'                                              !
!       'radlw_rrtm3_datatb.f'                                             !
!       'radlw_rrtm3_main.f'                                               !
!                                                                          !
!    the 'radlw_rrtm3_param.f' contains:                                   !
!                                                                          !
!       'module_radlw_parameters'  -- band parameters set up               !
!                                                                          !
!    the 'radlw_rrtm3_datatb.f' contains:                                  !
!                                                                          !
!       'module_radlw_avplank'     -- plank flux data                      !
!       'module_radlw_ref'         -- reference temperature and pressure   !
!       'module_radlw_cldprlw'     -- cloud property coefficients          !
!       'module_radlw_kgbnn'       -- absorption coeffients for 16         !
!                                     bands, where nn = 01-16              !
!                                                                          !
!    the 'radlw_rrtm3_main.f' contains:                                    !
!                                                                          !
!       'rrtmg_lw'        -- main lw radiation transfer                    !
!                                                                          !
!    in the main module 'rrtmg_lw' there are only two                      !
!    externally callable subroutines:                                      !
!                                                                          !
!                                                                          !
!       'lwrad'     -- main lw radiation routine                           !
!          inputs:                                                         !
!           (plyr,plvl,tlyr,tlvl,qlyr,olyr,gasvmr,                         !
!            clouds,icseed,aerosols,sfemis,sfgtmp,                         !
!            dzlyr,delpin,de_lgth,alpha,                                   !
!            npts, nlay, nlp1, lprnt,                                      !
!          outputs:                                                        !
!            hlwc,topflx,sfcflx,cldtau,                                    !
!!         optional outputs:                                               !
!            HLW0,HLWB,FLXPRF)                                             !
!                                                                          !
!       'rlwinit'   -- initialization routine                              !
!          inputs:                                                         !
!           ( me )                                                         !
!          outputs:                                                        !
!           (none)                                                         !
!                                                                          !
!    all the lw radiation subprograms become contained subprograms         !
!    in module 'rrtmg_lw' and many of them are not directly                !
!    accessable from places outside the module.                            !
!                                                                          !
!    derived data type constructs used:                                    !
!                                                                          !
!     1. radiation flux at toa: (from module 'module_radlw_parameters')    !
!          topflw_type   -  derived data type for toa rad fluxes           !
!            upfxc              total sky upward flux at toa               !
!            upfx0              clear sky upward flux at toa               !
!                                                                          !
!     2. radiation flux at sfc: (from module 'module_radlw_parameters')    !
!          sfcflw_type   -  derived data type for sfc rad fluxes           !
!            upfxc              total sky upward flux at sfc               !
!            upfx0              clear sky upward flux at sfc               !
!            dnfxc              total sky downward flux at sfc             !
!            dnfx0              clear sky downward flux at sfc             !
!                                                                          !
!     3. radiation flux profiles(from module 'module_radlw_parameters')    !
!          proflw_type    -  derived data type for rad vertical prof       !
!            upfxc              level upward flux for total sky            !
!            dnfxc              level downward flux for total sky          !
!            upfx0              level upward flux for clear sky            !
!            dnfx0              level downward flux for clear sky          !
!                                                                          !
!    external modules referenced:                                          !
!                                                                          !
!       'module physcons'                                                  !
!       'mersenne_twister'                                                 !
!                                                                          !
!    compilation sequence is:                                              !
!                                                                          !
!       'radlw_rrtm3_param.f'                                              !
!       'radlw_rrtm3_datatb.f'                                             !
!       'radlw_rrtm3_main.f'                                               !
!                                                                          !
!    and all should be put in front of routines that use lw modules        !
!                                                                          !
!==========================================================================!
!                                                                          !
!    the original aer program declarations:                                !
!                                                                          !
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!                                                                              !
! Copyright (c) 2002-2020, Atmospheric & Environmental Research, Inc. (AER)    !
! All rights reserved.                                                         !
!                                                                              !
! Redistribution and use in source and binary forms, with or without           !
! modification, are permitted provided that the following conditions are met:  !
!  * Redistributions of source code must retain the above copyright            !
!    notice, this list of conditions and the following disclaimer.             !
!  * Redistributions in binary form must reproduce the above copyright         !
!    notice, this list of conditions and the following disclaimer in the       !
!    documentation and/or other materials provided with the distribution.      !
!  * Neither the name of Atmospheric & Environmental Research, Inc., nor       !
!    the names of its contributors may be used to endorse or promote products  !
!    derived from this software without specific prior written permission.     !
!                                                                              !
! THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS"  !
! AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE    !
! IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE   !
! ARE DISCLAIMED. IN NO EVENT SHALL ATMOSPHERIC & ENVIRONMENTAL RESEARCH, INC.,!
! BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR       !
! CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF         !
! SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS     !
! INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN      !
! CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE)      !
! ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF       !
! THE POSSIBILITY OF SUCH DAMAGE.                                              !
!                        (http://www.rtweb.aer.com/)                           !
!                                                                              !
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!                                                                          !
! ************************************************************************ !
!                                                                          !
!                              rrtmg_lw                                    !
!                                                                          !
!                                                                          !
!                   a rapid radiative transfer model                       !
!                       for the longwave region                            !
!             for application to general circulation models                !
!                                                                          !
!                                                                          !
!            atmospheric and environmental research, inc.                  !
!                        131 hartwell avenue                               !
!                        lexington, ma 02421                               !
!                                                                          !
!                           eli j. mlawer                                  !
!                        jennifer s. delamere                              !
!                         michael j. iacono                                !
!                         shepard a. clough                                !
!                                                                          !
!                                                                          !
!                       email:  miacono@aer.com                            !
!                       email:  emlawer@aer.com                            !
!                       email:  jdelamer@aer.com                           !
!                                                                          !
!        the authors wish to acknowledge the contributions of the          !
!        following people:  steven j. taubman, karen cady-pereira,         !
!        patrick d. brown, ronald e. farren, luke chen, robert bergstrom.  !
!                                                                          !
! ************************************************************************ !
!                                                                          !
!    references:                                                           !
!    (rrtmg_lw/rrtm_lw):                                                   !
!      iacono, m.j., j.s. delamere, e.j. mlawer, m.w. shepard,             !
!      s.a. clough, and w.d collins, radiative forcing by long-lived       !
!      greenhouse gases: calculations with the aer radiative transfer      !
!      models, j, geophys. res., 113, d13103, doi:10.1029/2008jd009944,    !
!      2008.                                                               !
!                                                                          !
!      clough, s.a., m.w. shephard, e.j. mlawer, j.s. delamere,            !
!      m.j. iacono, k. cady-pereira, s. boukabara, and p.d. brown:         !
!      atmospheric radiative transfer modeling: a summary of the aer       !
!      codes, j. quant. spectrosc. radiat. transfer, 91, 233-244, 2005.    !
!                                                                          !
!      mlawer, e.j., s.j. taubman, p.d. brown, m.j. iacono, and s.a.       !
!      clough:  radiative transfer for inhomogeneous atmospheres: rrtm,    !
!      a validated correlated-k model for the longwave.  j. geophys. res., !
!      102, 16663-16682, 1997.                                             !
!                                                                          !
!    (mcica):                                                              !
!      pincus, r., h. w. barker, and j.-j. morcrette: a fast, flexible,    !
!      approximation technique for computing radiative transfer in         !
!      inhomogeneous cloud fields, j. geophys. res., 108(d13), 4376,       !
!      doi:10.1029/2002JD003322, 2003.                                     !
!                                                                          !
! ************************************************************************ !
!                                                                          !
!    aer's revision history:                                               !
!     this version of rrtmg_lw has been modified from rrtm_lw to use a     !
!     reduced set of g-points for application to gcms.                     !
!                                                                          !
! --  original version (derived from rrtm_lw), reduction of g-points,      !
!     other revisions for use with gcms.                                   !
!        1999: m. j. iacono, aer, inc.                                     !
! --  adapted for use with ncar/cam3.                                      !
!        may 2004: m. j. iacono, aer, inc.                                 !
! --  revised to add mcica capability.                                     !
!        nov 2005: m. j. iacono, aer, inc.                                 !
! --  conversion to f90 formatting for consistency with rrtmg_sw.          !
!        feb 2007: m. j. iacono, aer, inc.                                 !
! --  modifications to formatting to use assumed-shape arrays.             !
!        aug 2007: m. j. iacono, aer, inc.                                 !
!                                                                          !
! ************************************************************************ !
!                                                                          !
!    ncep modifications history log:                                       !
!                                                                          !
!       nov 1999,  ken campana       -- received the original code from    !
!                    aer (1998 ncar ccm version), updated to link up with  !
!                    ncep mrf model                                        !
!       jun 2000,  ken campana       -- added option to switch random and  !
!                    maximum/random cloud overlap                          !
!           2001,  shrinivas moorthi -- further updates for mrf model      !
!       may 2001,  yu-tai hou        -- updated on trace gases and cloud   !
!                    property based on rrtm_v3.0 codes.                    !
!       dec 2001,  yu-tai hou        -- rewritten code into fortran 90 std !
!                    set ncep radiation structure standard that contains   !
!                    three plug-in compatable fortran program files:       !
!                    'radlw_param.f', 'radlw_datatb.f', 'radlw_main.f'     !
!                    fixed bugs in subprograms taugb14, taugb2, etc. added !
!                    out-of-bounds protections. (a detailed note of        !
!                    up_to_date modifications/corrections by ncep was sent !
!                    to aer in 2002)                                       !
!       jun 2004,  yu-tai hou        -- added mike iacono's apr 2004       !
!                    modification of variable diffusivity angles.          !
!       apr 2005,  yu-tai hou        -- minor modifications on module      !
!                    structures include rain/snow effect (this version of  !
!                    code was given back to aer in jun 2006)               !
!       mar 2007,  yu-tai hou        -- added aerosol effect for ncep      !
!                    models using the generallized aerosol optical property!
!                    scheme for gfs model.                                 !
!       apr 2007,  yu-tai hou        -- added spectral band heating as an  !
!                    optional output to support the 500 km gfs model's     !
!                    upper stratospheric radiation calculations. and       !
!                    restructure optional outputs for easy access by       !
!                    different models.                                     !
!       oct 2008,  yu-tai hou        -- modified to include new features   !
!                    from aer's newer release v4.4-v4.7, including the     !
!                    mcica sub-grid cloud option. add rain/snow optical    !
!                    properties support to cloudy sky calculations.        !
!                    correct errors in mcica cloud optical properties for  !
!                    ebert & curry scheme (ilwcice=1) that needs band      !
!                    index conversion. simplified and unified sw and lw    !
!                    sub-column cloud subroutines into one module by using !
!                    optional parameters.                                  !
!       mar 2009,  yu-tai hou        -- replaced the original random number!
!                    generator coming from the original code with ncep w3  !
!                    library to simplify the program and moved sub-column  !
!                    cloud subroutines inside the main module. added       !
!                    option of user provided permutation seeds that could  !
!                    be randomly generated from forecast time stamp.       !
!       oct 2009,  yu-tai hou        -- modified subrtines "cldprop" and   !
!                    "rlwinit" according updats from aer's rrtmg_lw v4.8.  !
!       nov 2009,  yu-tai hou        -- modified subrtine "taumol" according
!                    updats from aer's rrtmg_lw version 4.82. notice the   !
!                    cloud ice/liquid are assumed as in-cloud quantities,  !
!                    not as grid averaged quantities.                      !
!       jun 2010,  yu-tai hou        -- optimized code to improve efficiency
!       apr 2012,  b. ferrier and y. hou -- added conversion factor to fu's!
!                    cloud-snow optical property scheme.                   !
!       nov 2012,  yu-tai hou        -- modified control parameters thru   !
!                     module 'physparam'.                                  !  
!       FEB 2017    A.Cheng   - add odpth output, effective radius input   !
!       jun 2018,  h-m lin/y-t hou   -- added new option of cloud overlap  !
!                     method 'de-correlation-length' for mcica application !
!                                                                          !
! ************************************************************************ !
!                                                                          !
!    additional aer revision history:                                      !
!       jul 2020,  m.j. iacono   -- added new mcica cloud overlap options  !
!                     exponential and exponential-random. each method can  !
!                     use either a constant or a latitude-varying and      !
!                     day-of-year varying decorrelation length selected    !
!                     with parameter "idcor".                              !
!                                                                          !
!!!!!  ==============================================================  !!!!!
!!!!!                         end descriptions                         !!!!!
!!!!!  ==============================================================  !!!!!
 
      module rrtmg_lw 
!
      use physcons,         only : con_g, con_cp, con_avgd, con_amd,    &
     &                             con_amw, con_amo3
      use mersenne_twister, only : random_setseed, random_number,       &
     &                             random_stat
      use machine,          only : kind_phys,                           &
     &                             im => kind_io4, rb => kind_phys,     &
     &                             kind_dbl_prec
 
      use module_radlw_parameters
!
      use module_radlw_avplank, only : totplnk
      use module_radlw_ref,     only : preflog, tref, chi_mls
!
      implicit none
!
      private
!
!  ...  version tag and last revision date
      character(40), parameter ::                                       &
     &   VTAGLW='NCEP LW v5.1  Nov 2012 -RRTMG-LW v4.82  '
!    &   VTAGLW='NCEP LW v5.0  Aug 2012 -RRTMG-LW v4.82  '
!    &   VTAGLW='RRTMG-LW v4.82  Nov 2009  '
!    &   VTAGLW='RRTMG-LW v4.8   Oct 2009  '
!    &   VTAGLW='RRTMG-LW v4.71  Mar 2009  '
!    &   VTAGLW='RRTMG-LW v4.4   Oct 2008  '
!    &   VTAGLW='RRTM-LW v2.3g   Mar 2007  '
!    &   VTAGLW='RRTM-LW v2.3g   Apr 2004  '
 
!  ---  constant values
      real (kind=kind_phys), parameter :: eps     = 1.0e-6
      real (kind=kind_phys), parameter :: oneminus= 1.0-eps
      real (kind=kind_phys), parameter :: cldmin  = tiny(cldmin)
      real (kind=kind_phys), parameter :: bpade   = 1.0/0.278  ! pade approx constant
      real (kind=kind_phys), parameter :: stpfac  = 296.0/1013.0
      real (kind=kind_phys), parameter :: wtdiff  = 0.5        ! weight for radiance to flux conversion
      real (kind=kind_phys), parameter :: tblint  = ntbl       ! lookup table conversion factor
      real (kind=kind_phys), parameter :: f_zero  = 0.0
      real (kind=kind_phys), parameter :: f_one   = 1.0
 
!  ...  atomic weights for conversion from mass to volume mixing ratios
      real (kind=kind_phys), parameter :: amdw    = con_amd/con_amw
      real (kind=kind_phys), parameter :: amdo3   = con_amd/con_amo3
 
!  ...  band indices
      integer, dimension(nbands) :: nspa, nspb
 
      data nspa / 1, 1, 9, 9, 9, 1, 9, 1, 9, 1, 1, 9, 9, 1, 9, 9 /
      data nspb / 1, 1, 5, 5, 5, 0, 1, 1, 1, 1, 1, 0, 0, 1, 0, 0 /
 
!  ...  band wavenumber intervals
!     real (kind=kind_phys) :: wavenum1(nbands), wavenum2(nbands)
!     data wavenum1/                                                    &
!    &         10.,  350.,  500.,  630.,  700.,  820.,  980., 1080.,    &
!err &       1180., 1390., 1480., 1800., 2080., 2250., 2390., 2600. /
!    &       1180., 1390., 1480., 1800., 2080., 2250., 2380., 2600. /
!     data wavenum2/                                                    &
!    &        350.,  500.,  630.,  700.,  820.,  980., 1080., 1180.,    &
!err &       1390., 1480., 1800., 2080., 2250., 2390., 2600., 3250. /
!    &       1390., 1480., 1800., 2080., 2250., 2380., 2600., 3250. /
!     real (kind=kind_phys) :: delwave(nbands)
!     data delwave / 340., 150., 130.,  70., 120., 160., 100., 100.,    &
!    &               210.,  90., 320., 280., 170., 130., 220., 650. /
 
!  ---  reset diffusivity angle for Bands 2-3 and 5-9 to vary (between 1.50
!       and 1.80) as a function of total column water vapor.  the function
!       has been defined to minimize flux and cooling rate errors in these bands
!       over a wide range of precipitable water values.
      real (kind=kind_phys), dimension(nbands) :: a0, a1, a2
 
      data a0 / 1.66,  1.55,  1.58,  1.66,  1.54, 1.454,  1.89,  1.33,  &
     &         1.668,  1.66,  1.66,  1.66,  1.66,  1.66,  1.66,  1.66 /
      data a1 / 0.00,  0.25,  0.22,  0.00,  0.13, 0.446, -0.10,  0.40,  &
     &        -0.006,  0.00,  0.00,  0.00,  0.00,  0.00,  0.00,  0.00 /
      data a2 / 0.00, -12.0, -11.7,  0.00, -0.72,-0.243,  0.19,-0.062,  &
     &         0.414,  0.00,  0.00,  0.00,  0.00,  0.00,  0.00,  0.00 /
 
!! ---  logical flags for optional output fields
 
      logical :: lhlwb  = .false.
      logical :: lhlw0  = .false.
      logical :: lflxprf= .false.
 
!  ---  those data will be set up only once by "rlwinit"
 
!  ...  fluxfac, heatfac are factors for fluxes (in w/m**2) and heating
!       rates (in k/day, or k/sec set by subroutine 'rlwinit')
!       semiss0 are default surface emissivity for each bands
 
      real (kind=kind_phys) :: fluxfac, heatfac, semiss0(nbands)
      data semiss0(:) / nbands*1.0 /
 
      real (kind=kind_phys) :: tau_tbl(0:ntbl)  
      real (kind=kind_phys) :: exp_tbl(0:ntbl)  
      real (kind=kind_phys) :: tfn_tbl(0:ntbl)  
 
!  ---  the following variables are used for sub-column cloud scheme
 
      integer, parameter :: ipsdlw0 = ngptlw     ! initial permutation seed
 
!  ---  public accessable subprograms
 
      public rrtmg_lw_run, rlwinit
 
 
! ================
      contains
! ================
 
 
      subroutine rrtmg_lw_run                                           &
     &     ( plyr,plvl,tlyr,tlvl,qlyr,olyr,gasvmr_co2, gasvmr_n2o,      &   !  ---  inputs
     &       gasvmr_ch4, gasvmr_o2, gasvmr_co, gasvmr_cfc11,            &
     &       gasvmr_cfc12, gasvmr_cfc22, gasvmr_ccl4,                   &
     &       icseed,aeraod,aerssa,sfemis,sfgtmp,                        &
     &       dzlyr,delpin,de_lgth,alpha,                                &
     &       npts, nlay, nlp1, lprnt, cld_cf, lslwr, top_at_1, iovr,    &
     &       iovr_rand, iovr_maxrand, iovr_max, iovr_dcorr, iovr_exp,   &
     &       iovr_exprand,                                              &
     &       inc_minor_gas, ilwcliq, ilwcice, isubclw,                  &
     &       hlwc,topflx,sfcflx,cldtau,                                 &   !  ---  outputs
     &       hlw0,hlwb,flxprf,                                          &   !  ---  optional
     &       cld_lwp, cld_ref_liq, cld_iwp, cld_ref_ice,                &
     &       cld_rwp,cld_ref_rain, cld_swp, cld_ref_snow,               &
     &       cld_od, errmsg, errflg                                     &
     &     )
 
!  ====================  defination of variables  ====================  !
!                                                                       !
!  input variables:                                                     !
!     plyr (npts,nlay) : layer mean pressures (mb)                      !
!     plvl (npts,nlp1) : interface pressures (mb)                       !
!     tlyr (npts,nlay) : layer mean temperature (k)                     !
!     tlvl (npts,nlp1) : interface temperatures (k)                     !
!     qlyr (npts,nlay) : layer specific humidity (gm/gm)   *see inside  !
!     olyr (npts,nlay) : layer ozone concentration (gm/gm) *see inside  !
!     gasvmr(npts,nlay,:): atmospheric gases amount:                    !
!                       (check module_radiation_gases for definition)   !
!       gasvmr(:,:,1)  -   co2 volume mixing ratio                      !
!       gasvmr(:,:,2)  -   n2o volume mixing ratio                      !
!       gasvmr(:,:,3)  -   ch4 volume mixing ratio                      !
!       gasvmr(:,:,4)  -   o2  volume mixing ratio                      !
!       gasvmr(:,:,5)  -   co  volume mixing ratio                      !
!       gasvmr(:,:,6)  -   cfc11 volume mixing ratio                    !
!       gasvmr(:,:,7)  -   cfc12 volume mixing ratio                    !
!       gasvmr(:,:,8)  -   cfc22 volume mixing ratio                    !
!       gasvmr(:,:,9)  -   ccl4  volume mixing ratio                    !
!     clouds(npts,nlay,:): layer cloud profiles:                        !
!                       (check module_radiation_clouds for definition)  !
!       clouds(:,:,1)  -   layer total cloud fraction                   !
!       clouds(:,:,2)  -   layer in-cloud liq water path   (g/m**2)     !
!       clouds(:,:,3)  -   mean eff radius for liq cloud   (micron)     !
!       clouds(:,:,4)  -   layer in-cloud ice water path   (g/m**2)     !
!       clouds(:,:,5)  -   mean eff radius for ice cloud   (micron)     !
!       clouds(:,:,6)  -   layer rain drop water path      (g/m**2)     !
!       clouds(:,:,7)  -   mean eff radius for rain drop   (micron)     !
!       clouds(:,:,8)  -   layer snow flake water path     (g/m**2)     !
!       clouds(:,:,9)  -   mean eff radius for snow flake  (micron)     !
!     icseed(npts)   : auxiliary special cloud related array            !
!                      when module variable isubclw=2, it provides      !
!                      permutation seed for each column profile that    !
!                      are used for generating random numbers.          !
!                      when isubclw /=2, it will not be used.           !
!     aerosols(npts,nlay,nbands,:) : aerosol optical properties         !
!                       (check module_radiation_aerosols for definition)!
!        (:,:,:,1)     - optical depth                                  !
!        (:,:,:,2)     - single scattering albedo                       !
!        (:,:,:,3)     - asymmetry parameter                            !
!     sfemis (npts)  : surface emissivity                               !
!     sfgtmp (npts)  : surface ground temperature (k)                   !
!     dzlyr(npts,nlay) : layer thickness (km)                           !
!     delpin(npts,nlay): layer pressure thickness (mb)                  !
!     de_lgth(npts)    : cloud decorrelation length (km)                !
!     alpha(npts,nlay) : EXP/ER cloud overlap decorrelation parameter   !
!     npts           : total number of horizontal points                !
!     nlay, nlp1     : total number of vertical layers, levels          !
!     lprnt          : cntl flag for diagnostic print out               !
!   inc_minor_gas - control flag for rare gases (ch4,n2o,o2,cfcs, etc.) !
!           =0: do not include rare gases                               !
!           >0: include all rare gases                                  !
!   ilwcliq - control flag for liq-cloud optical properties             !
!           =1: input cld liqp & reliq, hu & stamnes (1993)             !
!           =2: not used                                                !
!   ilwcice - control flag for ice-cloud optical properties             !
!           =1: input cld icep & reice, ebert & curry (1997)            !
!           =2: input cld icep & reice, streamer (1996)                 !
!           =3: input cld icep & reice, fu (1998)                       !
!   isubclw - sub-column cloud approximation control flag               !
!           =0: no sub-col cld treatment, use grid-mean cld quantities  !
!           =1: mcica sub-col, prescribed seeds to get random numbers   !
!           =2: mcica sub-col, providing array icseed for random numbers!
!   iovr  - clouds vertical overlapping control flag                    !
!           =iovr_rand                                                  !
!           =iovr_maxrand                                               !
!           =iovr_max                                                   !
!           =iovr_dcorr                                                 !
!           =iovr_exp                                                   !
!           =iovr_exprand                                               !
!   iovr_rand    - choice of cloud-overlap: random                      !
!   iovr_maxrand - choice of cloud-overlap: maximum random              !
!   iovr_max     - choice of cloud-overlap: maximum                     !
!   iovr_dcorr   - choice of cloud-overlap: decorrelation length        !
!   iovr_exp     - choice of cloud-overlap: exponential                 !
!   iovr_exprand - choice of cloud-overlap: exponential random          !
!                                                                       !
!  output variables:                                                    !
!     hlwc  (npts,nlay): total sky heating rate (k/day or k/sec)        !
!     topflx(npts)     : radiation fluxes at top, component:            !
!                        (check module_radlw_paramters for definition)  !
!        upfxc           - total sky upward flux at top (w/m2)          !
!        upfx0           - clear sky upward flux at top (w/m2)          !
!     sfcflx(npts)     : radiation fluxes at sfc, component:            !
!                        (check module_radlw_paramters for definition)  !
!        upfxc           - total sky upward flux at sfc (w/m2)          !
!        upfx0           - clear sky upward flux at sfc (w/m2)          !
!        dnfxc           - total sky downward flux at sfc (w/m2)        !
!        dnfx0           - clear sky downward flux at sfc (w/m2)        !
!     cldtau(npts,nlay): approx 10mu band layer cloud optical depth     !
!                                                                       !
!! optional output variables:                                           !
!     hlwb(npts,nlay,nbands): spectral band total sky heating rates     !
!     hlw0  (npts,nlay): clear sky heating rate (k/day or k/sec)        !
!     flxprf(npts,nlp1): level radiative fluxes (w/m2), components:     !
!                        (check module_radlw_paramters for definition)  !
!        upfxc           - total sky upward flux                        !
!        dnfxc           - total sky dnward flux                        !
!        upfx0           - clear sky upward flux                        !
!        dnfx0           - clear sky dnward flux                        !
!                                                                       !
!  module parameters, control variables:                                !
!     nbands           - number of longwave spectral bands              !
!     maxgas           - maximum number of absorbing gaseous            !
!     maxxsec          - maximum number of cross-sections               !
!     ngptlw           - total number of g-point subintervals           !
!     ng##             - number of g-points in band (##=1-16)           !
!     ngb(ngptlw)      - band indices for each g-point                  !
!     bpade            - pade approximation constant (1/0.278)          !
!     nspa,nspb(nbands)- number of lower/upper ref atm's per band       !
!     delwave(nbands)  - longwave band width (wavenumbers)              !
!     ipsdlw0          - permutation seed for mcica sub-col clds        !
!                                                                       !
!  major local variables:                                               !
!     pavel  (nlay)         - layer pressures (mb)                      !
!     delp   (nlay)         - layer pressure thickness (mb)             !
!     tavel  (nlay)         - layer temperatures (k)                    !
!     tz     (0:nlay)       - level (interface) temperatures (k)        !
!     semiss (nbands)       - surface emissivity for each band          !
!     wx     (nlay,maxxsec) - cross-section molecules concentration     !
!     coldry (nlay)         - dry air column amount                     !
!                                   (1.e-20*molecules/cm**2)            !
!     cldfrc (0:nlp1)       - layer cloud fraction                      !
!     taucld (nbands,nlay)  - layer cloud optical depth for each band   !
!     cldfmc (ngptlw,nlay)  - layer cloud fraction for each g-point     !
!     tauaer (nbands,nlay)  - aerosol optical depths                    !
!     fracs  (ngptlw,nlay)  - planck fractions                          !
!     tautot (ngptlw,nlay)  - total optical depths (gaseous+aerosols)   !
!     colamt (nlay,maxgas)  - column amounts of absorbing gases         !
!                             1-maxgas are for watervapor, carbon       !
!                             dioxide, ozone, nitrous oxide, methane,   !
!                             oxigen, carbon monoxide, respectively     !
!                             (molecules/cm**2)                         !
!     pwvcm                 - column precipitable water vapor (cm)      !
!     secdiff(nbands)       - variable diffusivity angle defined as     !
!                             an exponential function of the column     !
!                             water amount in bands 2-3 and 5-9.        !
!                             this reduces the bias of several w/m2 in  !
!                             downward surface flux in high water       !
!                             profiles caused by using the constant     !
!                             diffusivity angle of 1.66.         (mji)  !
!     facij  (nlay)         - indicator of interpolation factors        !
!                             =0/1: indicate lower/higher temp & height !
!     selffac(nlay)         - scale factor for self-continuum, equals   !
!                          (w.v. density)/(atm density at 296K,1013 mb) !
!     selffrac(nlay)        - factor for temp interpolation of ref      !
!                             self-continuum data                       !
!     indself(nlay)         - index of the lower two appropriate ref    !
!                             temp for the self-continuum interpolation !
!     forfac (nlay)         - scale factor for w.v. foreign-continuum   !
!     forfrac(nlay)         - factor for temp interpolation of ref      !
!                             w.v. foreign-continuum data               !
!     indfor (nlay)         - index of the lower two appropriate ref    !
!                             temp for the foreign-continuum interp     !
!     laytrop               - tropopause layer index at which switch is !
!                             made from one conbination kew species to  !
!                             another.                                  !
!     jp(nlay),jt(nlay),jt1(nlay)                                       !
!                           - lookup table indexes                      !
!     totuflux(0:nlay)      - total-sky upward longwave flux (w/m2)     !
!     totdflux(0:nlay)      - total-sky downward longwave flux (w/m2)   !
!     htr(nlay)             - total-sky heating rate (k/day or k/sec)   !
!     totuclfl(0:nlay)      - clear-sky upward longwave flux (w/m2)     !
!     totdclfl(0:nlay)      - clear-sky downward longwave flux (w/m2)   !
!     htrcl(nlay)           - clear-sky heating rate (k/day or k/sec)   !
!     fnet    (0:nlay)      - net longwave flux (w/m2)                  !
!     fnetc   (0:nlay)      - clear-sky net longwave flux (w/m2)        !
!                                                                       !
!                                                                       !
!  ======================    end of definitions    ===================  !
 
!  ---  inputs:
      integer, intent(in) :: npts, nlay, nlp1, ilwcliq, ilwcice,        &
           isubclw, iovr, iovr_dcorr, iovr_exp, iovr_exprand, iovr_rand,&
           iovr_maxrand, iovr_max
      integer, intent(in) :: icseed(npts)
 
      logical,  intent(in) :: lprnt, inc_minor_gas
 
      real (kind=kind_phys), dimension(:,:), intent(in) :: plvl,        &
     &       tlvl
      real (kind=kind_phys), dimension(:,:), intent(in) :: plyr,        &
     &       tlyr, qlyr, olyr, dzlyr, delpin
 
      real (kind=kind_phys),dimension(:,:),intent(in)::gasvmr_co2,      &
     &     gasvmr_n2o, gasvmr_ch4, gasvmr_o2, gasvmr_co, gasvmr_cfc11,  &
     &     gasvmr_cfc12, gasvmr_cfc22, gasvmr_ccl4
 
      real (kind=kind_phys), dimension(:,:),intent(in):: cld_cf
      real (kind=kind_phys), dimension(:,:),intent(in),optional::       &
     &       cld_lwp, cld_ref_liq,  cld_iwp, cld_ref_ice,               &
     &       cld_rwp, cld_ref_rain, cld_swp, cld_ref_snow,              &
     &       cld_od
 
      real (kind=kind_phys), dimension(:), intent(in) :: sfemis,        &
     &       sfgtmp, de_lgth
      real (kind=kind_phys), dimension(npts,nlay),intent(in) ::         &
             alpha
 
      real (kind=kind_phys), dimension(:,:,:),intent(in)::              &
     &       aeraod, aerssa
      logical, intent(in) :: lslwr, top_at_1
 
!  ---  outputs:
      real (kind=kind_phys), dimension(:,:), intent(inout) :: hlwc
      real (kind=kind_phys), dimension(:,:), intent(inout) ::           &
     &       cldtau
 
      type (topflw_type),    dimension(:), intent(inout) :: topflx
      type (sfcflw_type),    dimension(:), intent(inout) :: sfcflx
 
      character(len=*), intent(out) :: errmsg
      integer,          intent(out) :: errflg
 
!! ---  optional outputs:
      real (kind=kind_phys), dimension(:,:,:),optional,                 &
     &       intent(inout) :: hlwb
      real (kind=kind_phys), dimension(:,:),       optional,            &
     &       intent(inout) :: hlw0
      type (proflw_type),    dimension(:,:),       optional,            &
     &       intent(inout) :: flxprf
 
!  ---  locals:
      real (kind=kind_phys), dimension(0:nlp1) :: cldfrc
 
      real (kind=kind_phys), dimension(0:nlay) :: totuflux, totdflux,   &
     &       totuclfl, totdclfl, tz
 
      real (kind=kind_phys), dimension(nlay)   :: htr, htrcl
 
      real (kind=kind_phys), dimension(nlay)   :: pavel, tavel, delp,   &
     &       clwp, ciwp, relw, reiw, cda1, cda2, cda3, cda4,            &
     &       coldry, colbrd, h2ovmr, o3vmr, fac00, fac01, fac10, fac11, &
     &       selffac, selffrac, forfac, forfrac, minorfrac, scaleminor, &
     &       scaleminorn2, temcol, dz
 
      real (kind=kind_phys), dimension(nbands,0:nlay) :: pklev, pklay
 
      real (kind=kind_phys), dimension(nlay,nbands) :: htrb
      real (kind=kind_phys), dimension(nbands,nlay) :: taucld, tauaer
      real (kind=kind_phys), dimension(nbands,npts,nlay) :: taucld3
      real (kind=kind_phys), dimension(ngptlw,nlay) :: fracs, tautot
      real (kind=kind_phys), dimension(nlay,ngptlw) :: fracs_r
      real(kind=kind_phys), dimension(ngptlw,nlay) :: cldfmc
      real (kind=kind_phys), dimension(nbands) :: semiss, secdiff
 
!  ---  column amount of absorbing gases:
!       (:,m) m = 1-h2o, 2-co2, 3-o3, 4-n2o, 5-ch4, 6-o2, 7-co
      real (kind=kind_phys) :: colamt(nlay,maxgas)
 
!  ---  column cfc cross-section amounts:
!       (:,m) m = 1-ccl4, 2-cfc11, 3-cfc12, 4-cfc22
      real (kind=kind_phys) :: wx(nlay,maxxsec)
 
!  ---  reference ratios of binary species parameter in lower atmosphere:
!       (:,m,:) m = 1-h2o/co2, 2-h2o/o3, 3-h2o/n2o, 4-h2o/ch4, 5-n2o/co2, 6-o3/co2
      real (kind=kind_phys) :: rfrate(nlay,nrates,2)
 
      real (kind=kind_phys) :: tem0, tem1, tem2, pwvcm, summol, stemp,  &
     &                         delgth
      real (kind=kind_phys), dimension(nlay) :: alph
 
      integer, dimension(npts) :: ipseed
      integer, dimension(nlay) :: jp, jt, jt1, indself, indfor, indminor
      integer                  :: laytrop, iplon, i, j, k, k1
      integer                  :: ig
      integer                  :: inflglw, iceflglw, liqflglw
      logical :: lcf1
      integer :: istart              ! beginning band of calculation
      integer :: iend                ! ending band of calculation
      integer :: iout                ! output option flag (inactive)
 
 
!
!===> ... begin here
!
      ! Initialize CCPP error handling variables
      errmsg = ''
      errflg = 0
 
!mz*
! For passing in cloud physical properties; cloud optics parameterized
! in RRTMG:
      inflglw = 2
      iceflglw = 3
      liqflglw = 1
      istart = 1
      iend = 16
      iout = 0
 
!
      if (.not. lslwr) return
 
!  --- ...  initialization
 
      lhlwb  = present ( hlwb )
      lhlw0  = present ( hlw0 )
      lflxprf= present ( flxprf )
 
      colamt(:,:) = f_zero
      cldtau(:,:) = f_zero
 
!! --- check for optional input arguments, depending on cloud method
      if (ilwcliq > 0) then    ! use prognostic cloud method
        if ( .not.present(cld_lwp) .or. .not.present(cld_ref_liq) .or.  &
     &       .not.present(cld_iwp) .or. .not.present(cld_ref_ice) .or.  &
     &       .not.present(cld_rwp) .or. .not.present(cld_ref_rain) .or. &
     &       .not.present(cld_swp) .or. .not.present(cld_ref_snow)) then
          write(errmsg,'(*(a))')                                        &
     &               'Logic error: ilwcliq>0 requires the following',   &
     &               ' optional arguments to be present:',              &
     &               ' cld_lwp, cld_ref_liq, cld_iwp, cld_ref_ice,',    &
     &               ' cld_rwp, cld_ref_rain, cld_swp, cld_ref_snow'
          errflg = 1
          return
        end if
      else                     ! use diagnostic cloud method
        if ( .not.present(cld_od) ) then
          write(errmsg,'(*(a))')                                        &
     &               'Logic error: ilwcliq<=0 requires the following',  &
     &               ' optional argument to be present: cld_od'
          errflg = 1
          return
        end if
      endif                    ! end if_ilwcliq
 
 
      if     ( isubclw == 1 ) then     ! advance prescribed permutation seed
        do i = 1, npts
          ipseed(i) = ipsdlw0 + i
        enddo
      elseif ( isubclw == 2 ) then     ! use input array of permutation seeds
        do i = 1, npts
          ipseed(i) = icseed(i)
        enddo
      endif
 
!     if ( lprnt ) then
!       print *,'  In rrtmg_lw, isubclw, ipsdlw0,ipseed =',             &
!    &          isubclw, ipsdlw0, ipseed
!     endif
 
!  --- ...  loop over horizontal npts profiles
 
      lab_do_iplon : do iplon = 1, npts
 
        if (sfemis(iplon) > eps .and. sfemis(iplon) <= 1.0) then  ! input surface emissivity
          do j = 1, nbands
            semiss(j) = sfemis(iplon)
          enddo
        else                                                      ! use default values
          do j = 1, nbands
            semiss(j) = semiss0(j)
          enddo
        endif
 
        stemp = sfgtmp(iplon)          ! surface ground temp
        if (iovr == iovr_dcorr) delgth= de_lgth(iplon)    ! clouds decorr-length
 
!           the vertical index of internal array is from surface to top
 
!  --- ...  molecular amounts are input or converted to volume mixing ratio
!           and later then converted to molecular amount (molec/cm2) by the
!           dry air column coldry (in molec/cm2) which is calculated from the
!           layer pressure thickness (in mb), based on the hydrostatic equation
!  --- ...  and includes a correction to account for h2o in the layer.
 
        if (top_at_1) then       ! input from toa to sfc
 
          tem1 = 100.0 * con_g
          tem2 = 1.0e-20 * 1.0e3 * con_avgd
          tz(0) = tlvl(iplon,nlp1)
 
          do k = 1, nlay
            k1 = nlp1 - k
            pavel(k)= plyr(iplon,k1)
            delp(k) = delpin(iplon,k1)
            tavel(k)= tlyr(iplon,k1)
            tz(k)   = tlvl(iplon,k1)
            dz(k)   = dzlyr(iplon,k1)
            if (iovr == iovr_exp .or. iovr == iovr_exprand) alph(k) = alpha(iplon,k) ! alpha decorrelation
 
 
!test use
!           h2ovmr(k)= max(f_zero,qlyr(iplon,k1)*amdw)                  ! input mass mixing ratio
!           h2ovmr(k)= max(f_zero,qlyr(iplon,k1))                       ! input vol mixing ratio
!           o3vmr (k)= max(f_zero,olyr(iplon,k1))                       ! input vol mixing ratio
!ncep model use
            h2ovmr(k)= max(f_zero,qlyr(iplon,k1)                        &
     &                           *amdw/(f_one-qlyr(iplon,k1)))          ! input specific humidity
            o3vmr(k)= max(f_zero,olyr(iplon,k1)*amdo3)                 ! input mass mixing ratio
 
!  --- ...  tem0 is the molecular weight of moist air
            tem0 = (f_one - h2ovmr(k))*con_amd + h2ovmr(k)*con_amw
            coldry(k) = tem2*delp(k) / (tem1*tem0*(f_one+h2ovmr(k)))
            temcol(k) = 1.0e-12 * coldry(k)
 
            colamt(k,1) = max(f_zero,    coldry(k)*h2ovmr(k))          ! h2o
            colamt(k,2) = max(temcol(k), coldry(k)*gasvmr_co2(iplon,k1)) ! co2
            colamt(k,3) = max(temcol(k), coldry(k)*o3vmr(k))           ! o3
          enddo
 
 
          if (inc_minor_gas) then
            do k = 1, nlay
              k1 = nlp1 - k
              colamt(k,4)=max(temcol(k), coldry(k)*gasvmr_n2o(iplon,k1))  ! n2o
              colamt(k,5)=max(temcol(k), coldry(k)*gasvmr_ch4(iplon,k1))  ! ch4
              colamt(k,6)=max(f_zero,    coldry(k)*gasvmr_o2(iplon,k1))   ! o2
              colamt(k,7)=max(f_zero,    coldry(k)*gasvmr_co(iplon,k1))   ! co
 
              wx(k,1) = max( f_zero, coldry(k)*gasvmr_ccl4(iplon,k1) )    ! ccl4
              wx(k,2) = max( f_zero, coldry(k)*gasvmr_cfc11(iplon,k1) )   ! cf11
              wx(k,3) = max( f_zero, coldry(k)*gasvmr_cfc12(iplon,k1) )   ! cf12
              wx(k,4) = max( f_zero, coldry(k)*gasvmr_cfc22(iplon,k1) )   ! cf22
            enddo
          else
            do k = 1, nlay
              colamt(k,4) = f_zero     ! n2o
              colamt(k,5) = f_zero     ! ch4
              colamt(k,6) = f_zero     ! o2
              colamt(k,7) = f_zero     ! co
 
              wx(k,1) = f_zero
              wx(k,2) = f_zero
              wx(k,3) = f_zero
              wx(k,4) = f_zero
            enddo
          endif
 
 
          do k = 1, nlay
            k1 = nlp1 - k
            do j = 1, nbands
              tauaer(j,k) = aeraod(iplon,k1,j)                          &
     &                    * (f_one - aerssa(iplon,k1,j))
            enddo
          enddo
 
          if (ilwcliq > 0) then    ! use prognostic cloud method
            do k = 1, nlay
              k1 = nlp1 - k
              cldfrc(k)= cld_cf(iplon,k1)
              clwp(k)  = cld_lwp(iplon,k1)
              relw(k)  = cld_ref_liq(iplon,k1)
              ciwp(k)  = cld_iwp(iplon,k1)
              reiw(k)  = cld_ref_ice(iplon,k1)
              cda1(k)  = cld_rwp(iplon,k1)
              cda2(k)  = cld_ref_rain(iplon,k1)
              cda3(k)  = cld_swp(iplon,k1)
              cda4(k)  = cld_ref_snow(iplon,k1)
            enddo
          else                       ! use diagnostic cloud method
            do k = 1, nlay
              k1 = nlp1 - k
              cldfrc(k)= cld_cf(iplon,k1)
              cda1(k)  = cld_od(iplon,k1)
            enddo
          endif                      ! end if_ilwcliq
 
          cldfrc(0)    = f_one       ! padding value only
          cldfrc(nlp1) = f_zero      ! padding value only
 
 
          tem1 = f_zero
          tem2 = f_zero
          do k = 1, nlay
            tem1 = tem1 + coldry(k) + colamt(k,1)
            tem2 = tem2 + colamt(k,1)
          enddo
 
          tem0 = 10.0 * tem2 / (amdw * tem1 * con_g)
          pwvcm = tem0 * plvl(iplon,nlp1)
 
        else                        ! input from sfc to toa
 
          tem1 = 100.0 * con_g
          tem2 = 1.0e-20 * 1.0e3 * con_avgd
          tz(0) = tlvl(iplon,1)
 
          do k = 1, nlay
            pavel(k)= plyr(iplon,k)
            delp(k) = delpin(iplon,k)
            tavel(k)= tlyr(iplon,k)
            tz(k)   = tlvl(iplon,k+1)
            dz(k)   = dzlyr(iplon,k)
            if (iovr == iovr_exp .or. iovr == iovr_exprand) alph(k) = alpha(iplon,k) ! alpha decorrelation
 
!  --- ...  set absorber amount
!test use
!           h2ovmr(k)= max(f_zero,qlyr(iplon,k)*amdw)                   ! input mass mixing ratio
!           h2ovmr(k)= max(f_zero,qlyr(iplon,k))                        ! input vol mixing ratio
!           o3vmr (k)= max(f_zero,olyr(iplon,k))                        ! input vol mixing ratio
!ncep model use
            h2ovmr(k)= max(f_zero,qlyr(iplon,k)                         &
     &                           *amdw/(f_one-qlyr(iplon,k)))           ! input specific humidity
            o3vmr(k)= max(f_zero,olyr(iplon,k)*amdo3)                  ! input mass mixing ratio
 
!  --- ...  tem0 is the molecular weight of moist air
            tem0 = (f_one - h2ovmr(k))*con_amd + h2ovmr(k)*con_amw
            coldry(k) = tem2*delp(k) / (tem1*tem0*(f_one+h2ovmr(k)))
            temcol(k) = 1.0e-12 * coldry(k)
 
            colamt(k,1) = max(f_zero,    coldry(k)*h2ovmr(k))          ! h2o
            colamt(k,2) = max(temcol(k), coldry(k)*gasvmr_co2(iplon,k))! co2
            colamt(k,3) = max(temcol(k), coldry(k)*o3vmr(k))           ! o3
          enddo
 
!  --- ...  set up col amount for rare gases, convert from volume mixing ratio
!           to molec/cm2 based on coldry (scaled to 1.0e-20)
 
          if (inc_minor_gas) then
            do k = 1, nlay
              colamt(k,4)=max(temcol(k), coldry(k)*gasvmr_n2o(iplon,k))  ! n2o
              colamt(k,5)=max(temcol(k), coldry(k)*gasvmr_ch4(iplon,k))  ! ch4
              colamt(k,6)=max(f_zero,    coldry(k)*gasvmr_o2(iplon,k))   ! o2
              colamt(k,7)=max(f_zero,    coldry(k)*gasvmr_co(iplon,k))   ! co
 
              wx(k,1) = max( f_zero, coldry(k)*gasvmr_ccl4(iplon,k) )    ! ccl4
              wx(k,2) = max( f_zero, coldry(k)*gasvmr_cfc11(iplon,k) )   ! cf11
              wx(k,3) = max( f_zero, coldry(k)*gasvmr_cfc12(iplon,k) )   ! cf12
              wx(k,4) = max( f_zero, coldry(k)*gasvmr_cfc22(iplon,k) )   ! cf22
            enddo
          else
            do k = 1, nlay
              colamt(k,4) = f_zero     ! n2o
              colamt(k,5) = f_zero     ! ch4
              colamt(k,6) = f_zero     ! o2
              colamt(k,7) = f_zero     ! co
 
              wx(k,1) = f_zero
              wx(k,2) = f_zero
              wx(k,3) = f_zero
              wx(k,4) = f_zero
            enddo
          endif
 
!  --- ...  set aerosol optical properties
 
          do j = 1, nbands
            do k = 1, nlay
              tauaer(j,k) = aeraod(iplon,k,j)                           &
     &                    * (f_one - aerssa(iplon,k,j))
            enddo
          enddo
 
          if (ilwcliq > 0) then    ! use prognostic cloud method
            do k = 1, nlay
              cldfrc(k)= cld_cf(iplon,k)
              clwp(k)  = cld_lwp(iplon,k)
              relw(k)  = cld_ref_liq(iplon,k)
              ciwp(k)  = cld_iwp(iplon,k)
              reiw(k)  = cld_ref_ice(iplon,k)
              cda1(k)  = cld_rwp(iplon,k)
              cda2(k)  = cld_ref_rain(iplon,k)
              cda3(k)  = cld_swp(iplon,k)
              cda4(k)  = cld_ref_snow(iplon,k)
            enddo
          else                       ! use diagnostic cloud method
            do k = 1, nlay
              cldfrc(k)= cld_cf(iplon,k)
              cda1(k)  = cld_od(iplon,k)
            enddo
          endif                      ! end if_ilwcliq
 
          cldfrc(0)    = f_one       ! padding value only
          cldfrc(nlp1) = f_zero      ! padding value only
 
!  --- ...  compute precipitable water vapor for diffusivity angle adjustments
 
          tem1 = f_zero
          tem2 = f_zero
          do k = 1, nlay
            tem1 = tem1 + coldry(k) + colamt(k,1)
            tem2 = tem2 + colamt(k,1)
          enddo
 
          tem0 = 10.0 * tem2 / (amdw * tem1 * con_g)
          pwvcm = tem0 * plvl(iplon,1)
 
        endif                       ! top_at_1
 
 
        do k = 1, nlay
          summol = f_zero
          do i = 2, maxgas
            summol = summol + colamt(k,i)
          enddo
          colbrd(k) = coldry(k) - summol
        enddo
 
 
        tem1 = 1.80
        tem2 = 1.50
        do j = 1, nbands
          if (j==1 .or. j==4 .or. j==10) then
            secdiff(j) = 1.66
          else
            secdiff(j) = min( tem1, max( tem2,                          &
     &                   a0(j)+a1(j)*exp(a2(j)*pwvcm) ))
          endif
        enddo
 
!     if (lprnt) then
!      print *,'  coldry',coldry
!      print *,' wx(*,1) ',(wx(k,1),k=1,NLAY)
!      print *,' wx(*,2) ',(wx(k,2),k=1,NLAY)
!      print *,' wx(*,3) ',(wx(k,3),k=1,NLAY)
!      print *,' wx(*,4) ',(wx(k,4),k=1,NLAY)
!      print *,' iplon ',iplon
!      print *,'  pavel ',pavel
!      print *,'  delp ',delp
!      print *,'  tavel ',tavel
!      print *,'  tz ',tz
!      print *,' h2ovmr ',h2ovmr
!      print *,' o3vmr ',o3vmr
!     endif
 
 
        lcf1 = .false.
        lab_do_k0 : do k = 1, nlay
          if ( cldfrc(k) > eps ) then
            lcf1 = .true.
            exit lab_do_k0
          endif
        enddo  lab_do_k0
 
        if ( lcf1 ) then
 
          call cldprop                                                  &
!  ---  inputs:
     &     ( cldfrc,clwp,relw,ciwp,reiw,cda1,cda2,cda3,cda4,            &
     &       nlay, nlp1, ipseed(iplon), dz, delgth, iovr, alph,         &
     &       ilwcliq, ilwcice, isubclw,                                 &
!  ---  outputs:
     &       cldfmc, taucld                                             &
     &     )
 
!  --- ...  save computed layer cloud optical depth for output
!           rrtm band-7 is apprx 10mu channel (or use spectral mean of bands 6-8)
 
          if (top_at_1) then       ! input from toa to sfc
            do k = 1, nlay
              k1 = nlp1 - k
              cldtau(iplon,k1) = taucld( 7,k)
            enddo
          else                        ! input from sfc to toa
            do k = 1, nlay
              cldtau(iplon,k) = taucld( 7,k)
            enddo
          endif                       ! end if_top_at_1_block
 
        else
          cldfmc = f_zero
          taucld = f_zero
        endif
 
!     if (lprnt) then
!      print *,' after cldprop'
!      print *,' clwp',clwp
!      print *,' ciwp',ciwp
!      print *,' relw',relw
!      print *,' reiw',reiw
!      print *,' taucl',cda1
!      print *,' cldfrac',cldfrc
!     endif
 
        call setcoef                                                    &
!  ---  inputs:
     &     ( pavel,tavel,tz,stemp,h2ovmr,colamt,coldry,colbrd,          &
     &       nlay, nlp1,                                                &
!  ---  outputs:
     &       laytrop,pklay,pklev,jp,jt,jt1,                             &
     &       rfrate,fac00,fac01,fac10,fac11,                            &
     &       selffac,selffrac,indself,forfac,forfrac,indfor,            &
     &       minorfrac,scaleminor,scaleminorn2,indminor                 &
     &     )
 
!     if (lprnt) then
!      print *,'laytrop',laytrop
!      print *,'colh2o',(colamt(k,1),k=1,NLAY)
!      print *,'colco2',(colamt(k,2),k=1,NLAY)
!      print *,'colo3', (colamt(k,3),k=1,NLAY)
!      print *,'coln2o',(colamt(k,4),k=1,NLAY)
!      print *,'colch4',(colamt(k,5),k=1,NLAY)
!      print *,'fac00',fac00
!      print *,'fac01',fac01
!      print *,'fac10',fac10
!      print *,'fac11',fac11
!      print *,'jp',jp
!      print *,'jt',jt
!      print *,'jt1',jt1
!      print *,'selffac',selffac
!      print *,'selffrac',selffrac
!      print *,'indself',indself
!      print *,'forfac',forfac
!      print *,'forfrac',forfrac
!      print *,'indfor',indfor
!     endif
 
 
        call taumol                                                     &
!  ---  inputs:
     &     ( laytrop,pavel,coldry,colamt,colbrd,wx,tauaer,              &
     &       rfrate,fac00,fac01,fac10,fac11,jp,jt,jt1,                  &
     &       selffac,selffrac,indself,forfac,forfrac,indfor,            &
     &       minorfrac,scaleminor,scaleminorn2,indminor,                &
     &       nlay,                                                      &
!  ---  outputs:
     &       fracs, tautot                                              &
     &     )
 
!     if (lprnt) then
!     print *,' after taumol'
!     do k = 1, nlay
!       write(6,121) k
!121    format(' k =',i3,5x,'FRACS')
!       write(6,122) (fracs(j,k),j=1,ngptlw)
!122    format(10e14.7)
!       write(6,123) k
!123    format(' k =',i3,5x,'TAUTOT')
!       write(6,122) (tautot(j,k),j=1,ngptlw)
!     enddo
!     endif
 
 
        if (isubclw <= 0) then
 
          if (iovr <= 0) then
 
            call rtrn                                                   &
!  ---  inputs:
     &     ( semiss,delp,cldfrc,taucld,tautot,pklay,pklev,              &
     &       fracs,secdiff,nlay,nlp1,                                   &
!  ---  outputs:
     &       totuflux,totdflux,htr, totuclfl,totdclfl,htrcl, htrb       &
     &     )
 
          else
 
            call rtrnmr                                                 &
!  ---  inputs:
     &     ( semiss,delp,cldfrc,taucld,tautot,pklay,pklev,              &
     &       fracs,secdiff,nlay,nlp1,                                   &
!  ---  outputs:
     &       totuflux,totdflux,htr, totuclfl,totdclfl,htrcl, htrb       &
     &     )
 
          endif   ! end if_iovr_block
 
        else
 
          call rtrnmc                                                   &
!  ---  inputs:
     &     ( semiss,delp,cldfmc,taucld,tautot,pklay,pklev,              &
     &       fracs,secdiff,nlay,nlp1,                                   &
!  ---  outputs:
     &       totuflux,totdflux,htr, totuclfl,totdclfl,htrcl, htrb       &
     &     )
 
        endif   ! end if_isubclw_block
 
 
        topflx(iplon)%upfxc = totuflux(nlay)
        topflx(iplon)%upfx0 = totuclfl(nlay)
 
        sfcflx(iplon)%upfxc = totuflux(0)
        sfcflx(iplon)%upfx0 = totuclfl(0)
        sfcflx(iplon)%dnfxc = totdflux(0)
        sfcflx(iplon)%dnfx0 = totdclfl(0)
 
        if (top_at_1) then       ! output from toa to sfc
 
!! --- ...  optional fluxes
          if ( lflxprf ) then
            do k = 0, nlay
              k1 = nlp1 - k
              flxprf(iplon,k1)%upfxc = totuflux(k)
              flxprf(iplon,k1)%dnfxc = totdflux(k)
              flxprf(iplon,k1)%upfx0 = totuclfl(k)
              flxprf(iplon,k1)%dnfx0 = totdclfl(k)
            enddo
          endif
 
          do k = 1, nlay
            k1 = nlp1 - k
            hlwc(iplon,k1) = htr(k)
          enddo
 
!! --- ...  optional clear sky heating rate
          if ( lhlw0 ) then
            do k = 1, nlay
              k1 = nlp1 - k
              hlw0(iplon,k1) = htrcl(k)
            enddo
          endif
 
!! --- ...  optional spectral band heating rate
          if ( lhlwb ) then
            do j = 1, nbands
            do k = 1, nlay
              k1 = nlp1 - k
              hlwb(iplon,k1,j) = htrb(k,j)
            enddo
            enddo
          endif
 
        else                        ! output from sfc to toa
 
!! --- ...  optional fluxes
          if ( lflxprf ) then
            do k = 0, nlay
              flxprf(iplon,k+1)%upfxc = totuflux(k)
              flxprf(iplon,k+1)%dnfxc = totdflux(k)
              flxprf(iplon,k+1)%upfx0 = totuclfl(k)
              flxprf(iplon,k+1)%dnfx0 = totdclfl(k)
            enddo
          endif
 
          do k = 1, nlay
            hlwc(iplon,k) = htr(k)
          enddo
 
!! --- ...  optional clear sky heating rate
          if ( lhlw0 ) then
            do k = 1, nlay
              hlw0(iplon,k) = htrcl(k)
            enddo
          endif
 
!! --- ...  optional spectral band heating rate
          if ( lhlwb ) then
            do j = 1, nbands
            do k = 1, nlay
              hlwb(iplon,k,j) = htrb(k,j)
            enddo
            enddo
          endif
 
        endif                       ! if_top_at_1
 
      enddo  lab_do_iplon
 
!...................................
      end subroutine rrtmg_lw_run
!-----------------------------------
 
      subroutine rlwinit( me, rad_hr_units, inc_minor_gas, ilwcliq,     &
           isubclw, iovr, iovr_rand, iovr_maxrand, iovr_max, iovr_dcorr,&
           iovr_exp, iovr_exprand, errflg, errmsg )
 
!  ===================  program usage description  ===================  !
!                                                                       !
! purpose:  initialize non-varying module variables, conversion factors,!
! and look-up tables.                                                   !
!                                                                       !
! subprograms called:  none                                             !
!                                                                       !
!  ====================  defination of variables  ====================  !
!                                                                       !
!  inputs:                                                              !
!   me            - print control for parallel process                  !
!   rad_hr_units  - 1 for heating rates in units K/day. 2 for K/s       !
!   inc_minor_gas - flag to turn on/off minor gases in rrtmg            !
!   ilwcliq - liquid cloud optical properties contrl flag               !
!           =0: input cloud opt depth from diagnostic scheme            !
!           >0: input cwp,rew, and other cloud content parameters       !
!   isubclw - sub-column cloud approximation control flag               !
!           =0: no sub-col cld treatment, use grid-mean cld quantities  !
!           =1: mcica sub-col, prescribed seeds to get random numbers   !
!           =2: mcica sub-col, providing array icseed for random numbers!
!   iovr  - clouds vertical overlapping control flag                    !
!           =iovr_rand                                                  !
!           =iovr_maxrand                                               !
!           =iovr_max                                                   !
!           =iovr_dcorr                                                 !
!           =iovr_exp                                                   !
!           =iovr_exprand                                               !
!   iovr_rand    - choice of cloud-overlap: random                      !
!   iovr_maxrand - choice of cloud-overlap: maximum random              !
!   iovr_max     - choice of cloud-overlap: maximum                     !
!   iovr_dcorr   - choice of cloud-overlap: decorrelation length        !
!   iovr_exp     - choice of cloud-overlap: exponential                 !
!   iovr_exprand - choice of cloud-overlap: exponential random          !
!                                                                       !
!  outputs:                                                             !
!   errflg  - error flag                                                !
!   errmsg  - error message                                             !
!                                                                       !
!  *******************************************************************  !
!  original code description                                            !
!                                                                       !
!  original version:       michael j. iacono; july, 1998                !
!  first revision for ncar ccm:               september, 1998           !
!  second revision for rrtm_v3.0:             september, 2002           !
!                                                                       !
!  this subroutine performs calculations necessary for the initialization
!  of the longwave model.  lookup tables are computed for use in the lw !
!  radiative transfer, and input absorption coefficient data for each   !
!  spectral band are reduced from 256 g-point intervals to 140.         !
!                                                                       !
!  *******************************************************************  !
!                                                                       !
! definitions:                                                          !
!   arrays for 10000-point look-up tables:                              !
!   tau_tbl - clear-sky optical depth (used in cloudy radiative transfer!
!   exp_tbl - exponential lookup table for tansmittance                 !
!   tfn_tbl - tau transition function; i.e. the transition of the Planck!
!             function from that for the mean layer temperature to that !
!             for the layer boundary temperature as a function of optical
!             depth. the "linear in tau" method is used to make the table
!                                                                       !
!  *******************************************************************  !
!                                                                       !
!  ======================  end of description block  =================  !
 
!  ---  inputs:
      integer, intent(in) :: me, rad_hr_units, ilwcliq, isubclw, iovr,  &
           iovr_rand, iovr_maxrand, iovr_max, iovr_dcorr, iovr_exp,     &
           iovr_exprand
      logical, intent(in) :: inc_minor_gas
 
!  ---  outputs:
      character(len=*), intent(out) :: errmsg
      integer,          intent(out) :: errflg
 
!  ---  locals:
      real (kind=kind_phys), parameter :: expeps = 1.e-20
 
      real (kind=kind_phys) :: tfn, pival, explimit
 
      integer               :: i
 
!
!===> ... begin here
!
      ! Initialize error-handling
      errflg = 0
      errmsg = ''
 
      if ((iovr .ne. iovr_rand) .and. (iovr .ne. iovr_maxrand) .and.    &
          (iovr .ne. iovr_max)  .and. (iovr .ne. iovr_dcorr)   .and.    &
          (iovr .ne. iovr_exp)  .and. (iovr .ne. iovr_exprand)) then
         errflg = 1
         errmsg = 'ERROR(rlwinit): Error in specification of cloud overlap flag'
      endif
 
      if (me == 0) then
        print *,' - Using AER Longwave Radiation, Version: ', vtaglw
 
        if (inc_minor_gas) then
          print *,'   --- Include rare gases N2O, CH4, O2, CFCs ',      &
     &            'absorptions in LW'
        else
          print *,'   --- Rare gases effect is NOT included in LW'
        endif
 
        if ( isubclw == 0 ) then
          print *,'   --- Using standard grid average clouds, no ',     &
     &            'sub-column clouds approximation applied'
        elseif ( isubclw == 1 ) then
          print *,'   --- Using MCICA sub-colum clouds approximation ', &
     &            'with a prescribed sequence of permutation seeds'
        elseif ( isubclw == 2 ) then
          print *,'   --- Using MCICA sub-colum clouds approximation ', &
     &            'with provided input array of permutation seeds'
        endif
      endif
 
 
      semiss0(:) = f_one
 
 
      pival = 2.0 * asin(f_one)
      fluxfac = pival * 2.0d4
!     fluxfac = 62831.85307179586                   ! = 2 * pi * 1.0e4
 
      if (rad_hr_units == 1) then
!       heatfac = 8.4391
!       heatfac = con_g * 86400. * 1.0e-2 / con_cp  !   (in k/day)
        heatfac = con_g * 864.0 / con_cp            !   (in k/day)
      else
        heatfac = con_g * 1.0e-2 / con_cp           !   (in k/second)
      endif
 
 
      tau_tbl(0) = f_zero
      exp_tbl(0) = f_one
      tfn_tbl(0) = f_zero
 
      tau_tbl(ntbl) = 1.e10
      exp_tbl(ntbl) = expeps
      tfn_tbl(ntbl) = f_one
 
      explimit = aint( -log(tiny(exp_tbl(0))) )
 
      do i = 1, ntbl-1
!org    tfn = float(i) / float(ntbl)
!org    tau_tbl(i) = bpade * tfn / (f_one - tfn)
        tfn = real(i, kind_phys) / real(ntbl-i, kind_phys)
        tau_tbl(i) = bpade * tfn
        if (tau_tbl(i) >= explimit) then
          exp_tbl(i) = expeps
        else
          exp_tbl(i) = exp( -tau_tbl(i) )
        endif
 
        if (tau_tbl(i) < 0.06) then
          tfn_tbl(i) = tau_tbl(i) / 6.0
        else
          tfn_tbl(i) = f_one - 2.0*( (f_one / tau_tbl(i))               &
     &               - ( exp_tbl(i) / (f_one - exp_tbl(i)) ) )
        endif
      enddo
 
!...................................
      end subroutine rlwinit
!-----------------------------------
 
 
      subroutine cldprop                                                &
     &     ( cfrac,cliqp,reliq,cicep,reice,cdat1,cdat2,cdat3,cdat4,     & !  ---  inputs
     &       nlay, nlp1, ipseed, dz, de_lgth, iovr, alpha, ilwcliq,     &
     &       ilwcice, isubclw, cldfmc, taucld                           & !  ---  outputs
     &     )
 
!  ===================  program usage description  ===================  !
!                                                                       !
! purpose:  compute the cloud optical depth(s) for each cloudy layer    !
! and g-point interval.                                                 !
!                                                                       !
! subprograms called:  none                                             !
!                                                                       !
!  ====================  defination of variables  ====================  !
!                                                                       !
!  inputs:                                                       -size- !
!    cfrac - real, layer cloud fraction                          0:nlp1 !
!        .....  for ilwcliq > 0  (prognostic cloud sckeme)  - - -       !
!    cliqp - real, layer in-cloud liq water path (g/m**2)          nlay !
!    reliq - real, mean eff radius for liq cloud (micron)          nlay !
!    cicep - real, layer in-cloud ice water path (g/m**2)          nlay !
!    reice - real, mean eff radius for ice cloud (micron)          nlay !
!    cdat1 - real, layer rain drop water path  (g/m**2)            nlay !
!    cdat2 - real, effective radius for rain drop (microm)         nlay !
!    cdat3 - real, layer snow flake water path (g/m**2)            nlay !
!    cdat4 - real, effective radius for snow flakes (micron)       nlay !
!        .....  for ilwcliq = 0  (diagnostic cloud sckeme)  - - -       !
!    cdat1 - real, input cloud optical depth                       nlay !
!    cdat2 - real, layer cloud single scattering albedo            nlay !
!    cdat3 - real, layer cloud asymmetry factor                    nlay !
!    cdat4 - real, optional use                                    nlay !
!    cliqp - not used                                              nlay !
!    reliq - not used                                              nlay !
!    cicep - not used                                              nlay !
!    reice - not used                                              nlay !
!                                                                       !
!    dz     - real, layer thickness (km)                           nlay !
!    de_lgth- real, layer cloud decorrelation length (km)             1 !
!    alpha  - real, EXP/ER decorrelation parameter                 nlay !
!    nlay  - integer, number of vertical layers                      1  !
!    nlp1  - integer, number of vertical levels                      1  !
!    ipseed- permutation seed for generating random numbers (isubclw>0) !
!                                                                       !
!  outputs:                                                             !
!    cldfmc - real, cloud fraction for each sub-column       ngptlw*nlay!
!    taucld - real, cld opt depth for bands (non-mcica)      nbands*nlay!
!                                                                       !
!  explanation of the method for each value of ilwcliq, and ilwcice.    !
!    set up in module "module_radlw_cntr_para"                          !
!                                                                       !
!     ilwcliq=0  : input cloud optical property (tau, ssa, asy).        !
!                  (used for diagnostic cloud method)                   !
!     ilwcliq>0  : input cloud liq/ice path and effective radius, also  !
!                  require the user of 'ilwcice' to specify the method  !
!                  used to compute aborption due to water/ice parts.    !
!  ...................................................................  !
!                                                                       !
!     ilwcliq=1:   the water droplet effective radius (microns) is input!
!                  and the opt depths due to water clouds are computed  !
!                  as in hu and stamnes, j., clim., 6, 728-742, (1993). !
!                  the values for absorption coefficients appropriate for
!                  the spectral bands in rrtm have been obtained for a  !
!                  range of effective radii by an averaging procedure   !
!                  based on the work of j. pinto (private communication).
!                  linear interpolation is used to get the absorption   !
!                  coefficients for the input effective radius.         !
!                                                                       !
!     ilwcice=1:   the cloud ice path (g/m2) and ice effective radius   !
!                  (microns) are input and the optical depths due to ice!
!                  clouds are computed as in ebert and curry, jgr, 97,  !
!                  3831-3836 (1992).  the spectral regions in this work !
!                  have been matched with the spectral bands in rrtm to !
!                  as great an extent as possible:                      !
!                     e&c 1      ib = 5      rrtm bands 9-16            !
!                     e&c 2      ib = 4      rrtm bands 6-8             !
!                     e&c 3      ib = 3      rrtm bands 3-5             !
!                     e&c 4      ib = 2      rrtm band 2                !
!                     e&c 5      ib = 1      rrtm band 1                !
!     ilwcice=2:   the cloud ice path (g/m2) and ice effective radius   !
!                  (microns) are input and the optical depths due to ice!
!                  clouds are computed as in rt code, streamer v3.0     !
!                  (ref: key j., streamer user's guide, cooperative     !
!                  institute for meteorological satellite studies, 2001,!
!                  96 pp.) valid range of values for re are between 5.0 !
!                  and 131.0 micron.                                    !
!     ilwcice=3:   the ice generalized effective size (dge) is input and!
!                  the optical properties, are calculated as in q. fu,  !
!                  j. climate, (1998). q. fu provided high resolution   !
!                  tales which were appropriately averaged for the bands!
!                  in rrtm_lw. linear interpolation is used to get the  !
!                  coeff from the stored tables. valid range of values  !
!                  for deg are between 5.0 and 140.0 micron.            !
!                                                                       !
!  other cloud control module variables:                                !
!     isubclw =0: standard cloud scheme, no sub-col cloud approximation !
!             >0: mcica sub-col cloud scheme using ipseed as permutation!
!                 seed for generating rundom numbers                    !
!                                                                       !
!  ======================  end of description block  =================  !
!
      use module_radlw_cldprlw
 
!  ---  inputs:
      integer, intent(in) :: nlay, nlp1, ipseed, iovr, ilwcliq, ilwcice,&
           isubclw
 
      real (kind=kind_phys), dimension(0:nlp1), intent(in) :: cfrac
      real (kind=kind_phys), dimension(nlay),   intent(in) :: cliqp,    &
     &       reliq, cicep, reice, cdat1, cdat2, cdat3, cdat4, dz
      real (kind=kind_phys),                    intent(in) :: de_lgth
      real (kind=kind_phys), dimension(nlay),   intent(in) :: alpha
 
!  ---  outputs:
      real (kind=kind_phys), dimension(ngptlw,nlay),intent(out):: cldfmc
      real (kind=kind_phys), dimension(nbands,nlay),intent(out):: taucld
 
!  ---  locals:
      real (kind=kind_phys), dimension(nbands) :: tauliq, tauice
      real (kind=kind_phys), dimension(nlay)   :: cldf
 
      real (kind=kind_phys) :: dgeice, factor, fint, tauran, tausnw,    &
     &       cldliq, refliq, cldice, refice
 
      logical :: lcloudy(ngptlw,nlay)
      integer :: ia, ib, ig, k, index
 
!
!===> ...  begin here
!
      do k = 1, nlay
        do ib = 1, nbands
          taucld(ib,k) = f_zero
        enddo
      enddo
 
      do k = 1, nlay
        do ig = 1, ngptlw
          cldfmc(ig,k) = f_zero
        enddo
      enddo
 
 
!  --- ...  compute cloud radiative properties for a cloudy column
 
      lab_if_ilwcliq : if (ilwcliq > 0) then
 
        lab_do_k : do k = 1, nlay
          lab_if_cld : if (cfrac(k) > cldmin) then
 
            tauran = absrain * cdat1(k)                      ! ncar formula
!!          tausnw = abssnow1 * cdat3(k)                     ! ncar formula
!  ---  if use fu's formula it needs to be normalized by snow density
!       !not use snow density = 0.1 g/cm**3 = 0.1 g/(mu * m**2)
!       use ice density = 0.9167 g/cm**3 = 0.9167 g/(mu * m**2)
!       factor 1.5396=8/(3*sqrt(3)) converts reff to generalized ice particle size
!       use newer factor value 1.0315
!       1/(0.9167*1.0315) = 1.05756
            if (cdat3(k)>f_zero .and. cdat4(k)>10.0_kind_phys) then
              tausnw = abssnow0*1.05756*cdat3(k)/cdat4(k)      ! fu's formula
            else
              tausnw = f_zero
            endif
 
            cldliq = cliqp(k)
            cldice = cicep(k)
!           refliq = max(2.5e0, min(60.0e0, reliq(k) ))
!           refice = max(5.0e0, reice(k) )
            refliq = reliq(k)
            refice = reice(k)
 
!  --- ...  calculation of absorption coefficients due to water clouds.
 
            if ( cldliq <= f_zero ) then
              do ib = 1, nbands
                tauliq(ib) = f_zero
              enddo
            else
              if ( ilwcliq == 1 ) then
 
                factor = refliq - 1.5
                index  = max( 1, min( 57, int( factor ) ))
                fint   = factor - float(index)
 
                do ib = 1, nbands
                  tauliq(ib) = max(f_zero, cldliq*(absliq1(index,ib)    &
     &              + fint*(absliq1(index+1,ib)-absliq1(index,ib)) ))
                enddo
              endif   ! end if_ilwcliq_block
            endif   ! end if_cldliq_block
 
!  --- ...  calculation of absorption coefficients due to ice clouds.
 
            if ( cldice <= f_zero ) then
              do ib = 1, nbands
                tauice(ib) = f_zero
              enddo
            else
 
!  --- ...  ebert and curry approach for all particle sizes though somewhat
!           unjustified for large ice particles
 
              if ( ilwcice == 1 ) then
                refice = min(130.0, max(13.0, real(refice) ))
 
                do ib = 1, nbands
                  ia = ipat(ib)             ! eb_&_c band index for ice cloud coeff
                  tauice(ib) = max(f_zero, cldice*(absice1(1,ia)        &
     &                         + absice1(2,ia)/refice) )
                enddo
 
!  --- ...  streamer approach for ice effective radius between 5.0 and 131.0 microns
!           and ebert and curry approach for ice eff radius greater than 131.0 microns.
!           no smoothing between the transition of the two methods.
 
              elseif ( ilwcice == 2 ) then
 
                factor = (refice - 2.0) / 3.0
                index  = max( 1, min( 42, int( factor ) ))
                fint   = factor - float(index)
 
                do ib = 1, nbands
                  tauice(ib) = max(f_zero, cldice*(absice2(index,ib)    &
     &              + fint*(absice2(index+1,ib) - absice2(index,ib)) ))
                enddo
 
!  --- ...  fu's approach for ice effective radius between 4.8 and 135 microns
!           (generalized effective size from 5 to 140 microns)
 
              elseif ( ilwcice == 3 ) then
 
!               dgeice = max(5.0, 1.5396*refice)              ! v4.4 value
                dgeice = max(5.0, 1.0315*refice)              ! v4.71 value
                factor = (dgeice - 2.0) / 3.0
                index  = max( 1, min( 45, int( factor ) ))
                fint   = factor - float(index)
 
                do ib = 1, nbands
                  tauice(ib) = max(f_zero, cldice*(absice3(index,ib)    &
     &              + fint*(absice3(index+1,ib) - absice3(index,ib)) ))
                enddo
 
              endif   ! end if_ilwcice_block
            endif   ! end if_cldice_block
 
            do ib = 1, nbands
              taucld(ib,k) = tauice(ib) + tauliq(ib) + tauran + tausnw
            enddo
 
          endif  lab_if_cld
        enddo  lab_do_k
 
      else  lab_if_ilwcliq
 
        do k = 1, nlay
          if (cfrac(k) > cldmin) then
            do ib = 1, nbands
              taucld(ib,k) = cdat1(k)
            enddo
          endif
        enddo
 
      endif  lab_if_ilwcliq
 
 
      if ( isubclw > 0 ) then      ! mcica sub-col clouds approx
        do k = 1, nlay
          if ( cfrac(k) < cldmin ) then
            cldf(k) = f_zero
          else
            cldf(k) = cfrac(k)
          endif
        enddo
 
!  --- ...  call sub-column cloud generator
 
        call mcica_subcol                                               &
!  ---  inputs:
     &     ( cldf, nlay, ipseed, dz, de_lgth, alpha, iovr,              &
!  ---  output:
     &       lcloudy                                                    &
     &     )
 
        do k = 1, nlay
          do ig = 1, ngptlw
            if ( lcloudy(ig,k) ) then
              cldfmc(ig,k) = f_one
            else
              cldfmc(ig,k) = f_zero
            endif
          enddo
        enddo
 
      endif   ! end if_isubclw_block
 
! ..................................
      end subroutine cldprop
! ----------------------------------
 
      subroutine mcica_subcol                                           &
     &    ( cldf, nlay, ipseed, dz, de_lgth, alpha, iovr,               & !  ---  inputs
     &      lcloudy                                                     & !  ---  outputs
     &    )
 
!  ====================  defination of variables  ====================  !
!                                                                       !
!  input variables:                                                size !
!   cldf    - real, layer cloud fraction                           nlay !
!   nlay    - integer, number of model vertical layers               1  !
!   ipseed  - integer, permute seed for random num generator         1  !
!    ** note : if the cloud generator is called multiple times, need    !
!              to permute the seed between each call; if between calls  !
!              for lw and sw, use values differ by the number of g-pts. !
!   dz      - real, layer thickness (km)                           nlay !
!   de_lgth - real, layer cloud decorrelation length (km)            1  !
!   alpha   - real, EXP/ER decorrelation parameter                 nlay !
!   iovr    - control flag for cloud overlapping method              1  !
!                 =0:random; =1:maximum/random: =2:maximum; =3:decorr   !
!                 =4:exponential; =5:exponential-random                 !
!                                                                       !
!  output variables:                                                    !
!   lcloudy - logical, sub-colum cloud profile flag array    ngptlw*nlay!
!                                                                       !
!  =====================    end of definitions    ====================  !
 
      implicit none
 
!  ---  inputs:
      integer, intent(in) :: nlay, ipseed, iovr
 
      real (kind=kind_phys), dimension(nlay), intent(in) :: cldf, dz
      real (kind=kind_phys),                  intent(in) :: de_lgth
      real (kind=kind_phys), dimension(nlay), intent(in) :: alpha
 
!  ---  outputs:
      logical, dimension(ngptlw,nlay), intent(out) :: lcloudy
 
!  ---  locals:
      real (kind=kind_phys) :: cdfunc(ngptlw,nlay),                     &
     &                            tem1, fac_lcf(nlay),                  &
     &       cdfun2(ngptlw,nlay)
      real (kind=kind_dbl_prec) rand2d(nlay*ngptlw), rand1d(ngptlw)
 
      type (random_stat) :: stat          ! for thread safe random generator
 
      integer :: k, n, k1
!
!===> ...  begin here
!
 
      call random_setseed                                               &
!  ---  inputs:
     &    ( ipseed,                                                     &
!  ---  outputs:
     &      stat                                                        &
     &    )
 
 
      select case ( iovr )
 
        case( 0 )        ! random overlap, pick a random value at every level
 
          call random_number                                            &
!  ---  inputs: ( none )
!  ---  outputs:
     &     ( rand2d, stat )
 
          k1 = 0
          do n = 1, ngptlw
            do k = 1, nlay
              k1 = k1 + 1
              cdfunc(n,k) = rand2d(k1)
            enddo
          enddo
 
        case( 1 )        ! max-ran overlap
 
          call random_number                                            &
!  ---  inputs: ( none )
!  ---  outputs:
     &     ( rand2d, stat )
 
          k1 = 0
          do n = 1, ngptlw
            do k = 1, nlay
              k1 = k1 + 1
              cdfunc(n,k) = rand2d(k1)
            enddo
          enddo
 
!  ---  first pick a random number for bottom (or top) layer.
!       then walk up the column: (aer's code)
!       if layer below is cloudy, use the same rand num in the layer below
!       if layer below is clear,  use a new random number
 
!  ---  from bottom up
          do k = 2, nlay
            k1 = k - 1
            tem1 = f_one - cldf(k1)
 
            do n = 1, ngptlw
              if ( cdfunc(n,k1) > tem1 ) then
                cdfunc(n,k) = cdfunc(n,k1)
              else
                cdfunc(n,k) = cdfunc(n,k) * tem1
              endif
            enddo
          enddo
 
!  ---  or walk down the column: (if use original author's method)
!       if layer above is cloudy, use the same rand num in the layer above
!       if layer above is clear,  use a new random number
 
!  ---  from top down
!         do k = nlay-1, 1, -1
!           k1 = k + 1
!           tem1 = f_one - cldf(k1)
 
!           do n = 1, ngptlw
!             if ( cdfunc(n,k1) > tem1 ) then
!               cdfunc(n,k) = cdfunc(n,k1)
!             else
!               cdfunc(n,k) = cdfunc(n,k) * tem1
!             endif
!           enddo
!         enddo
 
        case( 2 )        
 
          call random_number                                            &
!  ---  inputs: ( none )
!  ---  outputs:
     &     ( rand1d, stat )
 
          do n = 1, ngptlw
            tem1 = rand1d(n)
 
            do k = 1, nlay
              cdfunc(n,k) = tem1
            enddo
          enddo
 
        case( 3 )        ! decorrelation length overlap
 
!  ---  compute overlapping factors based on layer midpoint distances
!       and decorrelation depths
 
          do k = nlay, 2, -1
            fac_lcf(k) = exp( -0.5 * (dz(k)+dz(k-1)) / de_lgth )
          enddo
 
!  ---  setup 2 sets of random numbers
 
          call random_number ( rand2d, stat )
 
          k1 = 0
          do k = 1, nlay
            do n = 1, ngptlw
              k1 = k1 + 1
              cdfunc(n,k) = rand2d(k1)
            enddo
          enddo
 
          call random_number ( rand2d, stat )
 
          k1 = 0
          do k = 1, nlay
            do n = 1, ngptlw
              k1 = k1 + 1
              cdfun2(n,k) = rand2d(k1)
            enddo
          enddo
 
!  ---  then working from the top down:
!       if a random number (from an independent set -cdfun2) is smaller then the
!       scale factor: use the upper layer's number,  otherwise use a new random
!       number (keep the original assigned one).
 
          do k = nlay-1, 1, -1
            k1 = k + 1
 
            do n = 1, ngptlw
              if ( cdfun2(n,k) <= fac_lcf(k1) ) then
                cdfunc(n,k) = cdfunc(n,k1)
              endif
            enddo
          enddo
 
        case( 4:5 )        ! exponential and exponential-random cloud overlap
 
!  ---  Use previously derived decorrelation parameter, alpha, to specify
!       the exponenential transition of cloud correlation in the vertical column.
!
!       For exponential cloud overlap, the correlation is applied across layers
!       without regard to the configuration of clear and cloudy layers.
 
!       For exponential-random cloud overlap, a new exponential transition is 
!       performed within each group of adjacent cloudy layers and blocks of 
!       cloudy layers with clear layers between them are correlated randomly. 
!
!       NOTE: The code below is identical for case (4) and (5) because the 
!       distinction in the vertical correlation between EXP and ER is already 
!       built into the specification of alpha (in subroutine get_alpha_exper). 
 
!  ---  setup 2 sets of random numbers
 
          call random_number ( rand2d, stat )
 
          k1 = 0
          do k = 1, nlay
            do n = 1, ngptlw
              k1 = k1 + 1
              cdfunc(n,k) = rand2d(k1)
            enddo
          enddo
 
          call random_number ( rand2d, stat )
 
          k1 = 0
          do k = 1, nlay
            do n = 1, ngptlw
              k1 = k1 + 1
              cdfun2(n,k) = rand2d(k1)
            enddo
          enddo
 
!  ---  then working upward from the surface:
!       if a random number (from an independent set: cdfun2) is smaller than 
!       alpha, then use the previous layer's number, otherwise use a new random
!       number (keep the originally assigned one in cdfunc for that layer).
 
          do k = 2, nlay
            k1 = k - 1
            do n = 1, ngptlw
              if ( cdfun2(n,k) < alpha(k) ) then
                   cdfunc(n,k) = cdfunc(n,k1)
              endif
            enddo
          enddo
 
      end select
 
 
      do k = 1, nlay
        tem1 = f_one - cldf(k)
 
        do n = 1, ngptlw
          lcloudy(n,k) = cdfunc(n,k) >= tem1
        enddo
      enddo
 
! ..................................
      end subroutine mcica_subcol
! ----------------------------------
 
      subroutine setcoef                                                &
     &     ( pavel,tavel,tz,stemp,h2ovmr,colamt,coldry,colbrd,          & !  ---  inputs:
     &       nlay, nlp1,                                                &
     &       laytrop,pklay,pklev,jp,jt,jt1,                             & !  ---  outputs:
     &       rfrate,fac00,fac01,fac10,fac11,                            &
     &       selffac,selffrac,indself,forfac,forfrac,indfor,            &
     &       minorfrac,scaleminor,scaleminorn2,indminor                 &
     &     )
 
!  ===================  program usage description  ===================  !
!                                                                       !
! purpose:  compute various coefficients needed in radiative transfer   !
!    calculations.                                                      !
!                                                                       !
! subprograms called:  none                                             !
!                                                                       !
!  ====================  defination of variables  ====================  !
!                                                                       !
!  inputs:                                                       -size- !
!   pavel     - real, layer pressures (mb)                         nlay !
!   tavel     - real, layer temperatures (k)                       nlay !
!   tz        - real, level (interface) temperatures (k)         0:nlay !
!   stemp     - real, surface ground temperature (k)                1   !
!   h2ovmr    - real, layer w.v. volum mixing ratio (kg/kg)        nlay !
!   colamt    - real, column amounts of absorbing gases      nlay*maxgas!
!                 2nd indices range: 1-maxgas, for watervapor,          !
!                 carbon dioxide, ozone, nitrous oxide, methane,        !
!                 oxigen, carbon monoxide,etc. (molecules/cm**2)        !
!   coldry    - real, dry air column amount                        nlay !
!   colbrd    - real, column amount of broadening gases            nlay !
!   nlay/nlp1 - integer, total number of vertical layers, levels    1   !
!                                                                       !
!  outputs:                                                             !
!   laytrop   - integer, tropopause layer index (unitless)          1   !
!   pklay     - real, integrated planck func at lay temp   nbands*0:nlay!
!   pklev     - real, integrated planck func at lev temp   nbands*0:nlay!
!   jp        - real, indices of lower reference pressure          nlay !
!   jt, jt1   - real, indices of lower reference temperatures      nlay !
!   rfrate    - real, ref ratios of binary species param   nlay*nrates*2!
!     (:,m,:)m=1-h2o/co2,2-h2o/o3,3-h2o/n2o,4-h2o/ch4,5-n2o/co2,6-o3/co2!
!     (:,:,n)n=1,2: the rates of ref press at the 2 sides of the layer  !
!   facij     - real, factors multiply the reference ks,           nlay !
!                 i,j=0/1 for lower/higher of the 2 appropriate         !
!                 temperatures and altitudes.                           !
!   selffac   - real, scale factor for w. v. self-continuum        nlay !
!                 equals (w. v. density)/(atmospheric density           !
!                 at 296k and 1013 mb)                                  !
!   selffrac  - real, factor for temperature interpolation of      nlay !
!                 reference w. v. self-continuum data                   !
!   indself   - integer, index of lower ref temp for selffac       nlay !
!   forfac    - real, scale factor for w. v. foreign-continuum     nlay !
!   forfrac   - real, factor for temperature interpolation of      nlay !
!                 reference w.v. foreign-continuum data                 !
!   indfor    - integer, index of lower ref temp for forfac        nlay !
!   minorfrac - real, factor for minor gases                       nlay !
!   scaleminor,scaleminorn2                                             !
!             - real, scale factors for minor gases                nlay !
!   indminor  - integer, index of lower ref temp for minor gases   nlay !
!                                                                       !
!  ======================    end of definitions    ===================  !
 
!  ---  inputs:
      integer, intent(in) :: nlay, nlp1
 
      real (kind=kind_phys), dimension(nlay,maxgas),intent(in):: colamt
      real (kind=kind_phys), dimension(0:nlay),     intent(in):: tz
 
      real (kind=kind_phys), dimension(nlay), intent(in) :: pavel,      &
     &       tavel, h2ovmr, coldry, colbrd
 
      real (kind=kind_phys), intent(in) :: stemp
 
!  ---  outputs:
      integer, dimension(nlay), intent(out) :: jp, jt, jt1, indself,    &
     &       indfor, indminor
 
      integer, intent(out) :: laytrop
 
      real (kind=kind_phys), dimension(nlay,nrates,2), intent(out) ::   &
     &       rfrate
      real (kind=kind_phys), dimension(nbands,0:nlay), intent(out) ::   &
     &       pklev, pklay
 
      real (kind=kind_phys), dimension(nlay),          intent(out) ::   &
     &       fac00, fac01, fac10, fac11, selffac, selffrac, forfac,     &
     &       forfrac, minorfrac, scaleminor, scaleminorn2
 
!  ---  locals:
      real (kind=kind_phys) :: tlvlfr, tlyrfr, plog, fp, ft, ft1,       &
     &       tem1, tem2
 
      integer :: i, k, jp1, indlev, indlay
!
!===> ... begin here
!
 
      indlay = min(180, max(1, int(stemp-159.0) ))
      indlev = min(180, max(1, int(tz(0)-159.0) ))
      tlyrfr = stemp - int(stemp)
      tlvlfr = tz(0) - int(tz(0))
      do i = 1, nbands
        tem1 = totplnk(indlay+1,i) - totplnk(indlay,i)
        tem2 = totplnk(indlev+1,i) - totplnk(indlev,i)
        pklay(i,0) = delwave(i) * (totplnk(indlay,i) + tlyrfr*tem1)
        pklev(i,0) = delwave(i) * (totplnk(indlev,i) + tlvlfr*tem2)
      enddo
 
!  --- ...  begin layer loop
 
      laytrop = 0
 
      do k = 1, nlay
 
        indlay = min(180, max(1, int(tavel(k)-159.0) ))
        tlyrfr = tavel(k) - int(tavel(k))
 
        indlev = min(180, max(1, int(tz(k)-159.0) ))
        tlvlfr = tz(k) - int(tz(k))
 
!  --- ...  begin spectral band loop
 
        do i = 1, nbands
          pklay(i,k) = delwave(i) * (totplnk(indlay,i) + tlyrfr         &
     &               * (totplnk(indlay+1,i) - totplnk(indlay,i)) )
          pklev(i,k) = delwave(i) * (totplnk(indlev,i) + tlvlfr         &
     &               * (totplnk(indlev+1,i) - totplnk(indlev,i)) )
        enddo
 
 
        plog = log(pavel(k))
        jp(k)= max(1, min(58, int(36.0 - 5.0*(plog+0.04)) ))
        jp1  = jp(k) + 1
!  --- ...  limit pressure extrapolation at the top
        fp   = max(f_zero, min(f_one, 5.0*(preflog(jp(k))-plog) ))
!org    fp   = 5.0 * (preflog(jp(k)) - plog)
 
 
        tem1 = (tavel(k)-tref(jp(k))) / 15.0
        tem2 = (tavel(k)-tref(jp1  )) / 15.0
        jt(k) = max(1, min(4, int(3.0 + tem1) ))
        jt1(k) = max(1, min(4, int(3.0 + tem2) ))
!  --- ...  restrict extrapolation ranges by limiting abs(det t) < 37.5 deg
        ft  = max(-0.5, min(1.5, tem1 - float(jt(k) - 3) ))
        ft1 = max(-0.5, min(1.5, tem2 - float(jt1(k) - 3) ))
!org    ft  = tem1 - float(jt (k) - 3)
!org    ft1 = tem2 - float(jt1(k) - 3)
 
 
        tem1 = f_one - fp
        fac10(k) = tem1 * ft
        fac00(k) = tem1 * (f_one - ft)
        fac11(k) = fp * ft1
        fac01(k) = fp * (f_one - ft1)
 
        forfac(k) = pavel(k)*stpfac / (tavel(k)*(1.0 + h2ovmr(k)))
        selffac(k) = h2ovmr(k) * forfac(k)
 
 
        scaleminor(k) = pavel(k) / tavel(k)
        scaleminorn2(k) = (pavel(k) / tavel(k))                         &
     &                  * (colbrd(k)/(coldry(k) + colamt(k,1)))
        tem1 = (tavel(k) - 180.8) / 7.2
        indminor(k) = min(18, max(1, int(tem1)))
        minorfrac(k) = tem1 - float(indminor(k))
 
 
        if (plog > 4.56) then
 
          laytrop =  laytrop + 1
 
          tem1 = (332.0 - tavel(k)) / 36.0
          indfor(k) = min(2, max(1, int(tem1)))
          forfrac(k) = tem1 - float(indfor(k))
 
 
          tem1 = (tavel(k) - 188.0) / 7.2
          indself(k) = min(9, max(1, int(tem1)-7))
          selffrac(k) = tem1 - float(indself(k) + 7)
 
 
          rfrate(k,1,1) = chi_mls(1,jp(k)) / chi_mls(2,jp(k))
          rfrate(k,1,2) = chi_mls(1,jp(k)+1) / chi_mls(2,jp(k)+1)
 
          rfrate(k,2,1) = chi_mls(1,jp(k)) / chi_mls(3,jp(k))
          rfrate(k,2,2) = chi_mls(1,jp(k)+1) / chi_mls(3,jp(k)+1)
 
          rfrate(k,3,1) = chi_mls(1,jp(k)) / chi_mls(4,jp(k))
          rfrate(k,3,2) = chi_mls(1,jp(k)+1) / chi_mls(4,jp(k)+1)
 
          rfrate(k,4,1) = chi_mls(1,jp(k)) / chi_mls(6,jp(k))
          rfrate(k,4,2) = chi_mls(1,jp(k)+1) / chi_mls(6,jp(k)+1)
 
          rfrate(k,5,1) = chi_mls(4,jp(k)) / chi_mls(2,jp(k))
          rfrate(k,5,2) = chi_mls(4,jp(k)+1) / chi_mls(2,jp(k)+1)
 
        else
 
          tem1 = (tavel(k) - 188.0) / 36.0
          indfor(k) = 3
          forfrac(k) = tem1 - f_one
 
          indself(k) = 0
          selffrac(k) = f_zero
 
 
          rfrate(k,1,1) = chi_mls(1,jp(k)) / chi_mls(2,jp(k))
          rfrate(k,1,2) = chi_mls(1,jp(k)+1) / chi_mls(2,jp(k)+1)
 
          rfrate(k,6,1) = chi_mls(3,jp(k)) / chi_mls(2,jp(k))
          rfrate(k,6,2) = chi_mls(3,jp(k)+1) / chi_mls(2,jp(k)+1)
 
        endif
 
 
        selffac(k) = colamt(k,1) * selffac(k)
        forfac(k)  = colamt(k,1) * forfac(k)
 
      enddo   ! end do_k layer loop
 
! ..................................
      end subroutine setcoef
! ----------------------------------
 
! ----------------------------------
      subroutine rtrn                                                   &
     &     ( semiss,delp,cldfrc,taucld,tautot,pklay,pklev,              & !  ---  inputs
     &       fracs,secdif, nlay,nlp1,                                   &
     &       totuflux,totdflux,htr, totuclfl,totdclfl,htrcl, htrb       & !  ---  outputs
     &     )
 
!  ===================  program usage description  ===================  !
!                                                                       !
! purpose:  compute the upward/downward radiative fluxes, and heating   !
! rates for both clear or cloudy atmosphere.  clouds are assumed as     !
! randomly overlaping in a vertical colum.                              !
!                                                                       !
! subprograms called:  none                                             !
!                                                                       !
!  ====================  defination of variables  ====================  !
!                                                                       !
!  inputs:                                                     -size-   !
!   semiss  - real, lw surface emissivity                         nbands!
!   delp    - real, layer pressure thickness (mb)                  nlay !
!   cldfrc  - real, layer cloud fraction                         0:nlp1 !
!   taucld  - real, layer cloud opt depth                    nbands,nlay!
!   tautot  - real, total optical depth (gas+aerosols)       ngptlw,nlay!
!   pklay   - real, integrated planck func at lay temp     nbands*0:nlay!
!   pklev   - real, integrated planck func at lev temp     nbands*0:nlay!
!   fracs   - real, planck fractions                         ngptlw,nlay!
!   secdif  - real, secant of diffusivity angle                   nbands!
!   nlay    - integer, number of vertical layers                    1   !
!   nlp1    - integer, number of vertical levels (interfaces)       1   !
!                                                                       !
!  outputs:                                                             !
!   totuflux- real, total sky upward flux (w/m2)                 0:nlay !
!   totdflux- real, total sky downward flux (w/m2)               0:nlay !
!   htr     - real, total sky heating rate (k/sec or k/day)        nlay !
!   totuclfl- real, clear sky upward flux (w/m2)                 0:nlay !
!   totdclfl- real, clear sky downward flux (w/m2)               0:nlay !
!   htrcl   - real, clear sky heating rate (k/sec or k/day)        nlay !
!   htrb    - real, spectral band lw heating rate (k/day)    nlay*nbands!
!                                                                       !
!  module veriables:                                                    !
!   ngb     - integer, band index for each g-value                ngptlw!
!   fluxfac - real, conversion factor for fluxes (pi*2.e4)           1  !
!   heatfac - real, conversion factor for heating rates (g/cp*1e-2)  1  !
!   tblint  - real, conversion factor for look-up tbl (float(ntbl)   1  !
!   bpade   - real, pade approx constant (1/0.278)                   1  !
!   wtdiff  - real, weight for radiance to flux conversion           1  !
!   ntbl    - integer, dimension of look-up tables                   1  !
!   tau_tbl - real, clr-sky opt dep lookup table                 0:ntbl !
!   exp_tbl - real, transmittance lookup table                   0:ntbl !
!   tfn_tbl - real, tau transition function                      0:ntbl !
!                                                                       !
!  local variables:                                                     !
!    itgas  - integer, index for gases contribution look-up table    1  !
!    ittot  - integer, index for gases plus clouds  look-up table    1  !
!    reflct - real, surface reflectance                              1  !
!    atrgas - real, gaseous absorptivity                             1  !
!    atrtot - real, gaseous and cloud absorptivity                   1  !
!    odcld  - real, cloud optical depth                              1  !
!    efclrfr- real, effective clear sky fraction (1-efcldfr)       nlay !
!    odepth - real, optical depth of gaseous only                    1  !
!    odtot  - real, optical depth of gas and cloud                   1  !
!    gasfac - real, gas-only pade factor, used for planck fn         1  !
!    totfac - real, gas+cld pade factor, used for planck fn          1  !
!    bbdgas - real, gas-only planck function for downward rt         1  !
!    bbugas - real, gas-only planck function for upward rt           1  !
!    bbdtot - real, gas and cloud planck function for downward rt    1  !
!    bbutot - real, gas and cloud planck function for upward rt      1  !
!    gassrcu- real, upwd source radiance due to gas only            nlay!
!    totsrcu- real, upwd source radiance due to gas+cld             nlay!
!    gassrcd- real, dnwd source radiance due to gas only             1  !
!    totsrcd- real, dnwd source radiance due to gas+cld              1  !
!    radtotu- real, spectrally summed total sky upwd radiance        1  !
!    radclru- real, spectrally summed clear sky upwd radiance        1  !
!    radtotd- real, spectrally summed total sky dnwd radiance        1  !
!    radclrd- real, spectrally summed clear sky dnwd radiance        1  !
!    toturad- real, total sky upward radiance by layer     0:nlay*nbands!
!    clrurad- real, clear sky upward radiance by layer     0:nlay*nbands!
!    totdrad- real, total sky downward radiance by layer   0:nlay*nbands!
!    clrdrad- real, clear sky downward radiance by layer   0:nlay*nbands!
!    fnet   - real, net longwave flux (w/m2)                     0:nlay !
!    fnetc  - real, clear sky net longwave flux (w/m2)           0:nlay !
!                                                                       !
!                                                                       !
!  *******************************************************************  !
!  original code description                                            !
!                                                                       !
!  original version:   e. j. mlawer, et al. rrtm_v3.0                   !
!  revision for gcms:  michael j. iacono; october, 2002                 !
!  revision for f90:   michael j. iacono; june, 2006                    !
!                                                                       !
!  this program calculates the upward fluxes, downward fluxes, and      !
!  heating rates for an arbitrary clear or cloudy atmosphere. the input !
!  to this program is the atmospheric profile, all Planck function      !
!  information, and the cloud fraction by layer.  a variable diffusivity!
!  angle (secdif) is used for the angle integration. bands 2-3 and 5-9  !
!  use a value for secdif that varies from 1.50 to 1.80 as a function   !
!  of the column water vapor, and other bands use a value of 1.66.  the !
!  gaussian weight appropriate to this angle (wtdiff=0.5) is applied    !
!  here.  note that use of the emissivity angle for the flux integration!
!  can cause errors of 1 to 4 W/m2 within cloudy layers.                !
!  clouds are treated with a random cloud overlap method.               !
!                                                                       !
!  *******************************************************************  !
!  ======================  end of description block  =================  !
 
!  ---  inputs:
      integer, intent(in) :: nlay, nlp1
 
      real (kind=kind_phys), dimension(0:nlp1), intent(in) :: cldfrc
      real (kind=kind_phys), dimension(nbands), intent(in) :: semiss,   &
     &       secdif
      real (kind=kind_phys), dimension(nlay),   intent(in) :: delp
 
      real (kind=kind_phys), dimension(nbands,nlay),intent(in):: taucld
      real (kind=kind_phys), dimension(ngptlw,nlay),intent(in):: fracs, &
     &       tautot
 
      real (kind=kind_phys), dimension(nbands,0:nlay), intent(in) ::    &
     &       pklev, pklay
 
!  ---  outputs:
      real (kind=kind_phys), dimension(nlay), intent(out) :: htr, htrcl
 
      real (kind=kind_phys), dimension(nlay,nbands),intent(out) :: htrb
 
      real (kind=kind_phys), dimension(0:nlay), intent(out) ::          &
     &       totuflux, totdflux, totuclfl, totdclfl
 
!  ---  locals:
      real (kind=kind_phys), parameter :: rec_6 = 0.166667
 
      real (kind=kind_phys), dimension(0:nlay,nbands) :: clrurad,       &
     &       clrdrad, toturad, totdrad
 
      real (kind=kind_phys), dimension(nlay)   :: gassrcu, totsrcu,     &
     &       trngas, efclrfr, rfdelp
      real (kind=kind_phys), dimension(0:nlay) :: fnet, fnetc
 
      real (kind=kind_phys) :: totsrcd, gassrcd, tblind, odepth, odtot, &
     &       odcld, atrtot, atrgas, reflct, totfac, gasfac, flxfac,     &
     &       plfrac, blay, bbdgas, bbdtot, bbugas, bbutot, dplnku,      &
     &       dplnkd, radtotu, radclru, radtotd, radclrd, rad0,          &
     &       clfr, trng, gasu
 
      integer :: ittot, itgas, ib, ig, k
!
!===> ...  begin here
!
      do ib = 1, nbands
        do k = 0, nlay
          toturad(k,ib) = f_zero
          totdrad(k,ib) = f_zero
          clrurad(k,ib) = f_zero
          clrdrad(k,ib) = f_zero
        enddo
      enddo
 
      do k = 0, nlay
        totuflux(k) = f_zero
        totdflux(k) = f_zero
        totuclfl(k) = f_zero
        totdclfl(k) = f_zero
      enddo
 
!  --- ...  loop over all g-points
 
      do ig = 1, ngptlw
        ib = ngb(ig)
 
        radtotd = f_zero
        radclrd = f_zero
 
 
        do k = nlay, 1, -1
 
!!\n  - clear sky, gases contribution
 
          odepth = max( f_zero, secdif(ib)*tautot(ig,k) )
          if (odepth <= 0.06) then
            atrgas = odepth - 0.5*odepth*odepth
            trng   = f_one - atrgas
            gasfac = rec_6 * odepth
          else
            tblind = odepth / (bpade + odepth)
            itgas = tblint*tblind + 0.5
            trng  = exp_tbl(itgas)
            atrgas = f_one - trng
            gasfac = tfn_tbl(itgas)
            odepth = tau_tbl(itgas)
          endif
 
          plfrac = fracs(ig,k)
          blay = pklay(ib,k)
 
          dplnku = pklev(ib,k  ) - blay
          dplnkd = pklev(ib,k-1) - blay
          bbdgas = plfrac * (blay + dplnkd*gasfac)
          bbugas = plfrac * (blay + dplnku*gasfac)
          gassrcd= bbdgas * atrgas
          gassrcu(k)= bbugas * atrgas
          trngas(k) = trng
 
!!\n  - total sky, gases+clouds contribution
 
          clfr = cldfrc(k)
          if (clfr >= eps) then
!!\n  - cloudy layer
 
            odcld = secdif(ib) * taucld(ib,k)
            efclrfr(k) = f_one-(f_one - exp(-odcld))*clfr
            odtot = odepth + odcld
            if (odtot < 0.06) then
              totfac = rec_6 * odtot
              atrtot = odtot - 0.5*odtot*odtot
            else
              tblind = odtot / (bpade + odtot)
              ittot  = tblint*tblind + 0.5
              totfac = tfn_tbl(ittot)
              atrtot = f_one - exp_tbl(ittot)
            endif
 
            bbdtot = plfrac * (blay + dplnkd*totfac)
            bbutot = plfrac * (blay + dplnku*totfac)
            totsrcd= bbdtot * atrtot
            totsrcu(k)= bbutot * atrtot
 
!  --- ...  total sky radiance
            radtotd = radtotd*trng*efclrfr(k) + gassrcd                 &
     &              + clfr*(totsrcd - gassrcd)
            totdrad(k-1,ib) = totdrad(k-1,ib) + radtotd
 
!  --- ...  clear sky radiance
            radclrd = radclrd*trng + gassrcd
            clrdrad(k-1,ib) = clrdrad(k-1,ib) + radclrd
 
          else
!  --- ...  clear layer
 
!  --- ...  total sky radiance
            radtotd = radtotd*trng + gassrcd
            totdrad(k-1,ib) = totdrad(k-1,ib) + radtotd
 
!  --- ...  clear sky radiance
            radclrd = radclrd*trng + gassrcd
            clrdrad(k-1,ib) = clrdrad(k-1,ib) + radclrd
 
          endif   ! end if_clfr_block
 
        enddo   ! end do_k_loop
 
 
!     note: spectral and Lambertian reflection are identical for the
!           diffusivity angle flux integration used here.
 
        reflct = f_one - semiss(ib)
        rad0 = semiss(ib) * fracs(ig,1) * pklay(ib,0)
 
        radtotu = rad0 + reflct*radtotd
        toturad(0,ib) = toturad(0,ib) + radtotu
 
        radclru = rad0 + reflct*radclrd
        clrurad(0,ib) = clrurad(0,ib) + radclru
 
 
        do k = 1, nlay
          clfr = cldfrc(k)
          trng = trngas(k)
          gasu = gassrcu(k)
 
          if (clfr >= eps) then
!  --- ...  cloudy layer
 
!  --- ... total sky radiance
            radtotu = radtotu*trng*efclrfr(k) + gasu                    &
     &            + clfr*(totsrcu(k) - gasu)
            toturad(k,ib) = toturad(k,ib) + radtotu
 
!  --- ... clear sky radiance
            radclru = radclru*trng + gasu
            clrurad(k,ib) = clrurad(k,ib) + radclru
 
          else
!  --- ...  clear layer
 
!  --- ... total sky radiance
            radtotu = radtotu*trng + gasu
            toturad(k,ib) = toturad(k,ib) + radtotu
 
!  --- ... clear sky radiance
            radclru = radclru*trng + gasu
            clrurad(k,ib) = clrurad(k,ib) + radclru
 
          endif   ! end if_clfr_block
 
        enddo   ! end do_k_loop
 
      enddo   ! end do_ig_loop
 
 
      flxfac = wtdiff * fluxfac
 
      do k = 0, nlay
        do ib = 1, nbands
          totuflux(k) = totuflux(k) + toturad(k,ib)
          totdflux(k) = totdflux(k) + totdrad(k,ib)
          totuclfl(k) = totuclfl(k) + clrurad(k,ib)
          totdclfl(k) = totdclfl(k) + clrdrad(k,ib)
        enddo
 
        totuflux(k) = totuflux(k) * flxfac
        totdflux(k) = totdflux(k) * flxfac
        totuclfl(k) = totuclfl(k) * flxfac
        totdclfl(k) = totdclfl(k) * flxfac
      enddo
 
!  --- ...  calculate net fluxes and heating rates
      fnet(0) = totuflux(0) - totdflux(0)
 
      do k = 1, nlay
        rfdelp(k) = heatfac / delp(k)
        fnet(k) = totuflux(k) - totdflux(k)
        htr(k) = (fnet(k-1) - fnet(k)) * rfdelp(k)
      enddo
 
!! --- ...  optional clear sky heating rates
      if ( lhlw0 ) then
        fnetc(0) = totuclfl(0) - totdclfl(0)
 
        do k = 1, nlay
          fnetc(k) = totuclfl(k) - totdclfl(k)
          htrcl(k) = (fnetc(k-1) - fnetc(k)) * rfdelp(k)
        enddo
      endif
 
!! --- ...  optional spectral band heating rates
      if ( lhlwb ) then
        do ib = 1, nbands
          fnet(0) = (toturad(0,ib) - totdrad(0,ib)) * flxfac
 
          do k = 1, nlay
            fnet(k) = (toturad(k,ib) - totdrad(k,ib)) * flxfac
            htrb(k,ib) = (fnet(k-1) - fnet(k)) * rfdelp(k)
          enddo
        enddo
      endif
 
! ..................................
      end subroutine rtrn
! ----------------------------------
 
 
! ----------------------------------
      subroutine rtrnmr                                                 &
     &     ( semiss,delp,cldfrc,taucld,tautot,pklay,pklev,              &!  ---  inputs
     &       fracs,secdif, nlay,nlp1,                                   &
     &       totuflux,totdflux,htr, totuclfl,totdclfl,htrcl, htrb       &  !  ---  outputs:
     &     )
 
!  ===================  program usage description  ===================  !
!                                                                       !
! purpose:  compute the upward/downward radiative fluxes, and heating   !
! rates for both clear or cloudy atmosphere.  clouds are assumed as in  !
! maximum-randomly overlaping in a vertical colum.                      !
!                                                                       !
! subprograms called:  none                                             !
!                                                                       !
!  ====================  defination of variables  ====================  !
!                                                                       !
!  inputs:                                                     -size-   !
!   semiss  - real, lw surface emissivity                         nbands!
!   delp    - real, layer pressure thickness (mb)                  nlay !
!   cldfrc  - real, layer cloud fraction                         0:nlp1 !
!   taucld  - real, layer cloud opt depth                    nbands,nlay!
!   tautot  - real, total optical depth (gas+aerosols)       ngptlw,nlay!
!   pklay   - real, integrated planck func at lay temp     nbands*0:nlay!
!   pklev   - real, integrated planck func at lev temp     nbands*0:nlay!
!   fracs   - real, planck fractions                         ngptlw,nlay!
!   secdif  - real, secant of diffusivity angle                   nbands!
!   nlay    - integer, number of vertical layers                    1   !
!   nlp1    - integer, number of vertical levels (interfaces)       1   !
!                                                                       !
!  outputs:                                                             !
!   totuflux- real, total sky upward flux (w/m2)                 0:nlay !
!   totdflux- real, total sky downward flux (w/m2)               0:nlay !
!   htr     - real, total sky heating rate (k/sec or k/day)        nlay !
!   totuclfl- real, clear sky upward flux (w/m2)                 0:nlay !
!   totdclfl- real, clear sky downward flux (w/m2)               0:nlay !
!   htrcl   - real, clear sky heating rate (k/sec or k/day)        nlay !
!   htrb    - real, spectral band lw heating rate (k/day)    nlay*nbands!
!                                                                       !
!  module veriables:                                                    !
!   ngb     - integer, band index for each g-value                ngptlw!
!   fluxfac - real, conversion factor for fluxes (pi*2.e4)           1  !
!   heatfac - real, conversion factor for heating rates (g/cp*1e-2)  1  !
!   tblint  - real, conversion factor for look-up tbl (float(ntbl)   1  !
!   bpade   - real, pade approx constant (1/0.278)                   1  !
!   wtdiff  - real, weight for radiance to flux conversion           1  !
!   ntbl    - integer, dimension of look-up tables                   1  !
!   tau_tbl - real, clr-sky opt dep lookup table                 0:ntbl !
!   exp_tbl - real, transmittance lookup table                   0:ntbl !
!   tfn_tbl - real, tau transition function                      0:ntbl !
!                                                                       !
!  local variables:                                                     !
!    itgas  - integer, index for gases contribution look-up table    1  !
!    ittot  - integer, index for gases plus clouds  look-up table    1  !
!    reflct - real, surface reflectance                              1  !
!    atrgas - real, gaseous absorptivity                             1  !
!    atrtot - real, gaseous and cloud absorptivity                   1  !
!    odcld  - real, cloud optical depth                              1  !
!    odepth - real, optical depth of gaseous only                    1  !
!    odtot  - real, optical depth of gas and cloud                   1  !
!    gasfac - real, gas-only pade factor, used for planck fn         1  !
!    totfac - real, gas+cld pade factor, used for planck fn          1  !
!    bbdgas - real, gas-only planck function for downward rt         1  !
!    bbugas - real, gas-only planck function for upward rt           1  !
!    bbdtot - real, gas and cloud planck function for downward rt    1  !
!    bbutot - real, gas and cloud planck function for upward rt      1  !
!    gassrcu- real, upwd source radiance due to gas only            nlay!
!    totsrcu- real, upwd source radiance due to gas + cld           nlay!
!    gassrcd- real, dnwd source radiance due to gas only             1  !
!    totsrcd- real, dnwd source radiance due to gas + cld            1  !
!    radtotu- real, spectrally summed total sky upwd radiance        1  !
!    radclru- real, spectrally summed clear sky upwd radiance        1  !
!    radtotd- real, spectrally summed total sky dnwd radiance        1  !
!    radclrd- real, spectrally summed clear sky dnwd radiance        1  !
!    toturad- real, total sky upward radiance by layer     0:nlay*nbands!
!    clrurad- real, clear sky upward radiance by layer     0:nlay*nbands!
!    totdrad- real, total sky downward radiance by layer   0:nlay*nbands!
!    clrdrad- real, clear sky downward radiance by layer   0:nlay*nbands!
!    fnet   - real, net longwave flux (w/m2)                     0:nlay !
!    fnetc  - real, clear sky net longwave flux (w/m2)           0:nlay !
!                                                                       !
!                                                                       !
!  *******************************************************************  !
!  original code description                                            !
!                                                                       !
!  original version:   e. j. mlawer, et al. rrtm_v3.0                   !
!  revision for gcms:  michael j. iacono; october, 2002                 !
!  revision for f90:   michael j. iacono; june, 2006                    !
!                                                                       !
!  this program calculates the upward fluxes, downward fluxes, and      !
!  heating rates for an arbitrary clear or cloudy atmosphere. the input !
!  to this program is the atmospheric profile, all Planck function      !
!  information, and the cloud fraction by layer.  a variable diffusivity!
!  angle (secdif) is used for the angle integration. bands 2-3 and 5-9  !
!  use a value for secdif that varies from 1.50 to 1.80 as a function   !
!  of the column water vapor, and other bands use a value of 1.66.  the !
!  gaussian weight appropriate to this angle (wtdiff=0.5) is applied    !
!  here.  note that use of the emissivity angle for the flux integration!
!  can cause errors of 1 to 4 W/m2 within cloudy layers.                !
!  clouds are treated with a maximum-random cloud overlap method.       !
!                                                                       !
!  *******************************************************************  !
!  ======================  end of description block  =================  !
 
!  ---  inputs:
      integer, intent(in) :: nlay, nlp1
 
      real (kind=kind_phys), dimension(0:nlp1), intent(in) :: cldfrc
      real (kind=kind_phys), dimension(nbands), intent(in) :: semiss,   &
     &       secdif
      real (kind=kind_phys), dimension(nlay),   intent(in) :: delp
 
      real (kind=kind_phys), dimension(nbands,nlay),intent(in):: taucld
      real (kind=kind_phys), dimension(ngptlw,nlay),intent(in):: fracs, &
     &       tautot
 
      real (kind=kind_phys), dimension(nbands,0:nlay), intent(in) ::    &
     &       pklev, pklay
 
!  ---  outputs:
      real (kind=kind_phys), dimension(nlay), intent(out) :: htr, htrcl
 
      real (kind=kind_phys), dimension(nlay,nbands),intent(out) :: htrb
 
      real (kind=kind_phys), dimension(0:nlay), intent(out) ::          &
     &       totuflux, totdflux, totuclfl, totdclfl
 
!  ---  locals:
      real (kind=kind_phys), parameter :: rec_6 = 0.166667
 
      real (kind=kind_phys), dimension(0:nlay,nbands) :: clrurad,       &
     &       clrdrad, toturad, totdrad
 
      real (kind=kind_phys), dimension(nlay)   :: gassrcu, totsrcu,     &
     &       trngas, trntot, rfdelp
      real (kind=kind_phys), dimension(0:nlay) :: fnet, fnetc
 
      real (kind=kind_phys) :: totsrcd, gassrcd, tblind, odepth, odtot, &
     &       odcld, atrtot, atrgas, reflct, totfac, gasfac, flxfac,     &
     &       plfrac, blay, bbdgas, bbdtot, bbugas, bbutot, dplnku,      &
     &       dplnkd, radtotu, radclru, radtotd, radclrd, rad0, rad,     &
     &       totradd, clrradd, totradu, clrradu, fmax, fmin, rat1, rat2,&
     &       radmod, clfr, trng, trnt, gasu, totu
 
      integer :: ittot, itgas, ib, ig, k
 
!  dimensions for cloud overlap adjustment
      real (kind=kind_phys), dimension(nlp1) :: faccld1u, faccld2u,     &
     &        facclr1u, facclr2u, faccmb1u, faccmb2u
      real (kind=kind_phys), dimension(0:nlay) :: faccld1d, faccld2d,   &
     &        facclr1d, facclr2d, faccmb1d, faccmb2d
 
      logical :: lstcldu(nlay), lstcldd(nlay)
!
!===> ...  begin here
!
      do k = 1, nlp1
        faccld1u(k) = f_zero
        faccld2u(k) = f_zero
        facclr1u(k) = f_zero
        facclr2u(k) = f_zero
        faccmb1u(k) = f_zero
        faccmb2u(k) = f_zero
      enddo
 
      lstcldu(1) = cldfrc(1) > eps
      rat1 = f_zero
      rat2 = f_zero
 
      do k = 1, nlay-1
 
        lstcldu(k+1) = cldfrc(k+1)>eps .and. cldfrc(k)<=eps
 
        if (cldfrc(k) > eps) then
 
 
          if (cldfrc(k+1) >= cldfrc(k)) then
            if (lstcldu(k)) then
              if (cldfrc(k) < f_one) then
                facclr2u(k+1) = (cldfrc(k+1) - cldfrc(k))               &
     &                        / (f_one - cldfrc(k))
              endif
              facclr2u(k) = f_zero
              faccld2u(k) = f_zero
            else
              fmax = max(cldfrc(k), cldfrc(k-1))
              if (cldfrc(k+1) > fmax) then
                facclr1u(k+1) = rat2
                facclr2u(k+1) = (cldfrc(k+1) - fmax)/(f_one - fmax)
              elseif (cldfrc(k+1) < fmax) then
                facclr1u(k+1) = (cldfrc(k+1) - cldfrc(k))               &
     &                        / (cldfrc(k-1) - cldfrc(k))
              else
                facclr1u(k+1) = rat2
              endif
            endif
 
            if (facclr1u(k+1)>f_zero .or. facclr2u(k+1)>f_zero) then
              rat1 = f_one
              rat2 = f_zero
            else
              rat1 = f_zero
              rat2 = f_zero
            endif
          else
            if (lstcldu(k)) then
              faccld2u(k+1) = (cldfrc(k) - cldfrc(k+1)) / cldfrc(k)
              facclr2u(k) = f_zero
              faccld2u(k) = f_zero
            else
              fmin = min(cldfrc(k), cldfrc(k-1))
              if (cldfrc(k+1) <= fmin) then
                faccld1u(k+1) = rat1
                faccld2u(k+1) = (fmin - cldfrc(k+1)) / fmin
              else
                faccld1u(k+1) = (cldfrc(k) - cldfrc(k+1))               &
     &                        / (cldfrc(k) - fmin)
              endif
            endif
 
            if (faccld1u(k+1)>f_zero .or. faccld2u(k+1)>f_zero) then
              rat1 = f_zero
              rat2 = f_one
            else
              rat1 = f_zero
              rat2 = f_zero
            endif
          endif
 
          faccmb1u(k+1) = facclr1u(k+1) * faccld2u(k) * cldfrc(k-1)
          faccmb2u(k+1) = faccld1u(k+1) * facclr2u(k)                   &
     &                  * (f_one - cldfrc(k-1))
        endif
 
      enddo
 
      do k = 0, nlay
        faccld1d(k) = f_zero
        faccld2d(k) = f_zero
        facclr1d(k) = f_zero
        facclr2d(k) = f_zero
        faccmb1d(k) = f_zero
        faccmb2d(k) = f_zero
      enddo
 
      lstcldd(nlay) = cldfrc(nlay) > eps
      rat1 = f_zero
      rat2 = f_zero
 
      do k = nlay, 2, -1
 
        lstcldd(k-1) = cldfrc(k-1) > eps .and. cldfrc(k)<=eps
 
        if (cldfrc(k) > eps) then
 
          if (cldfrc(k-1) >= cldfrc(k)) then
            if (lstcldd(k)) then
              if (cldfrc(k) < f_one) then
                facclr2d(k-1) = (cldfrc(k-1) - cldfrc(k))               &
     &                        / (f_one - cldfrc(k))
              endif
 
              facclr2d(k) = f_zero
              faccld2d(k) = f_zero
            else
              fmax = max(cldfrc(k), cldfrc(k+1))
 
              if (cldfrc(k-1) > fmax) then
                facclr1d(k-1) = rat2
                facclr2d(k-1) = (cldfrc(k-1) - fmax) / (f_one - fmax)
              elseif (cldfrc(k-1) < fmax) then
                facclr1d(k-1) = (cldfrc(k-1) - cldfrc(k))               &
     &                        / (cldfrc(k+1) - cldfrc(k))
              else
                facclr1d(k-1) = rat2
              endif
            endif
 
            if (facclr1d(k-1)>f_zero .or. facclr2d(k-1)>f_zero) then
              rat1 = f_one
              rat2 = f_zero
            else
              rat1 = f_zero
              rat2 = f_zero
            endif
          else
            if (lstcldd(k)) then
              faccld2d(k-1) = (cldfrc(k) - cldfrc(k-1)) / cldfrc(k)
              facclr2d(k) = f_zero
              faccld2d(k) = f_zero
            else
              fmin = min(cldfrc(k), cldfrc(k+1))
 
              if (cldfrc(k-1) <= fmin) then
                faccld1d(k-1) = rat1
                faccld2d(k-1) = (fmin - cldfrc(k-1)) / fmin
              else
                faccld1d(k-1) = (cldfrc(k) - cldfrc(k-1))               &
     &                        / (cldfrc(k) - fmin)
              endif
            endif
 
            if (faccld1d(k-1)>f_zero .or. faccld2d(k-1)>f_zero) then
              rat1 = f_zero
              rat2 = f_one
            else
              rat1 = f_zero
              rat2 = f_zero
            endif
          endif
 
          faccmb1d(k-1) = facclr1d(k-1) * faccld2d(k) * cldfrc(k+1)
          faccmb2d(k-1) = faccld1d(k-1) * facclr2d(k)                   &
     &                  * (f_one - cldfrc(k+1))
        endif
 
      enddo
 
 
      do ib = 1, nbands
        do k = 0, nlay
          toturad(k,ib) = f_zero
          totdrad(k,ib) = f_zero
          clrurad(k,ib) = f_zero
          clrdrad(k,ib) = f_zero
        enddo
      enddo
 
      do k = 0, nlay
        totuflux(k) = f_zero
        totdflux(k) = f_zero
        totuclfl(k) = f_zero
        totdclfl(k) = f_zero
      enddo
 
!  --- ...  loop over all g-points
 
      do ig = 1, ngptlw
        ib = ngb(ig)
 
        radtotd = f_zero
        radclrd = f_zero
 
 
        do k = nlay, 1, -1
 
!  --- ...  clear sky, gases contribution
 
          odepth = max( f_zero, secdif(ib)*tautot(ig,k) )
          if (odepth <= 0.06) then
            atrgas = odepth - 0.5*odepth*odepth
            trng   = f_one - atrgas
            gasfac = rec_6 * odepth
          else
            tblind = odepth / (bpade + odepth)
            itgas = tblint*tblind + 0.5
            trng  = exp_tbl(itgas)
            atrgas = f_one - trng
            gasfac = tfn_tbl(itgas)
            odepth = tau_tbl(itgas)
          endif
 
          plfrac = fracs(ig,k)
          blay = pklay(ib,k)
 
          dplnku = pklev(ib,k  ) - blay
          dplnkd = pklev(ib,k-1) - blay
          bbdgas = plfrac * (blay + dplnkd*gasfac)
          bbugas = plfrac * (blay + dplnku*gasfac)
          gassrcd   = bbdgas * atrgas
          gassrcu(k)= bbugas * atrgas
          trngas(k) = trng
 
!  --- ...  total sky, gases+clouds contribution
 
          clfr = cldfrc(k)
          if (lstcldd(k)) then
            totradd = clfr * radtotd
            clrradd = radtotd - totradd
            rad = f_zero
          endif
 
          if (clfr >= eps) then
 
            odcld = secdif(ib) * taucld(ib,k)
            odtot = odepth + odcld
            if (odtot < 0.06) then
              totfac = rec_6 * odtot
              atrtot = odtot - 0.5*odtot*odtot
              trnt   = f_one - atrtot
            else
              tblind = odtot / (bpade + odtot)
              ittot  = tblint*tblind + 0.5
              totfac = tfn_tbl(ittot)
              trnt   = exp_tbl(ittot)
              atrtot = f_one - trnt
            endif
 
            bbdtot = plfrac * (blay + dplnkd*totfac)
            bbutot = plfrac * (blay + dplnku*totfac)
            totsrcd   = bbdtot * atrtot
            totsrcu(k)= bbutot * atrtot
            trntot(k) = trnt
 
            totradd = totradd*trnt + clfr*totsrcd
            clrradd = clrradd*trng + (f_one - clfr)*gassrcd
 
            radtotd = totradd + clrradd
            totdrad(k-1,ib) = totdrad(k-1,ib) + radtotd
 
            radclrd = radclrd*trng + gassrcd
            clrdrad(k-1,ib) = clrdrad(k-1,ib) + radclrd
 
            radmod = rad*(facclr1d(k-1)*trng + faccld1d(k-1)*trnt)      &
     &             - faccmb1d(k-1)*gassrcd + faccmb2d(k-1)*totsrcd
 
            rad = -radmod + facclr2d(k-1)*(clrradd + radmod)            &
     &                    - faccld2d(k-1)*(totradd - radmod)
            totradd = totradd + rad
            clrradd = clrradd - rad
 
          else
!  --- ...  clear layer
 
!  --- ...  total sky radiance
            radtotd = radtotd*trng + gassrcd
            totdrad(k-1,ib) = totdrad(k-1,ib) + radtotd
 
!  --- ...  clear sky radiance
            radclrd = radclrd*trng + gassrcd
            clrdrad(k-1,ib) = clrdrad(k-1,ib) + radclrd
 
          endif   ! end if_clfr_block
 
        enddo   ! end do_k_loop
 
 
!     note: spectral and Lambertian reflection are identical for the
!           diffusivity angle flux integration used here.
 
        reflct = f_one - semiss(ib)
        rad0 = semiss(ib) * fracs(ig,1) * pklay(ib,0)
 
        radtotu = rad0 + reflct*radtotd
        toturad(0,ib) = toturad(0,ib) + radtotu
 
        radclru = rad0 + reflct*radclrd
        clrurad(0,ib) = clrurad(0,ib) + radclru
 
 
        do k = 1, nlay
 
          clfr = cldfrc(k)
          trng = trngas(k)
          gasu = gassrcu(k)
 
          if (lstcldu(k)) then
            totradu = clfr * radtotu
            clrradu = radtotu - totradu
            rad = f_zero
          endif
 
          if (clfr >= eps) then
 
            trnt = trntot(k)
            totu = totsrcu(k)
            totradu = totradu*trnt + clfr*totu
            clrradu = clrradu*trng + (f_one - clfr)*gasu
 
            radtotu = totradu + clrradu
            toturad(k,ib) = toturad(k,ib) + radtotu
 
            radclru = radclru*trng + gasu
            clrurad(k,ib) = clrurad(k,ib) + radclru
 
            radmod = rad*(facclr1u(k+1)*trng + faccld1u(k+1)*trnt)      &
     &             - faccmb1u(k+1)*gasu + faccmb2u(k+1)*totu
            rad = -radmod + facclr2u(k+1)*(clrradu + radmod)            &
     &                    - faccld2u(k+1)*(totradu - radmod)
            totradu = totradu + rad
            clrradu = clrradu - rad
 
          else
!  --- ...  clear layer
 
!  --- ...  total sky radiance
            radtotu = radtotu*trng + gasu
            toturad(k,ib) = toturad(k,ib) + radtotu
 
!  --- ...  clear sky radiance
            radclru = radclru*trng + gasu
            clrurad(k,ib) = clrurad(k,ib) + radclru
 
          endif   ! end if_clfr_block
 
        enddo   ! end do_k_loop
 
      enddo   ! end do_ig_loop
 
 
      flxfac = wtdiff * fluxfac
 
      do k = 0, nlay
        do ib = 1, nbands
          totuflux(k) = totuflux(k) + toturad(k,ib)
          totdflux(k) = totdflux(k) + totdrad(k,ib)
          totuclfl(k) = totuclfl(k) + clrurad(k,ib)
          totdclfl(k) = totdclfl(k) + clrdrad(k,ib)
        enddo
 
        totuflux(k) = totuflux(k) * flxfac
        totdflux(k) = totdflux(k) * flxfac
        totuclfl(k) = totuclfl(k) * flxfac
        totdclfl(k) = totdclfl(k) * flxfac
      enddo
 
!  --- ...  calculate net fluxes and heating rates
      fnet(0) = totuflux(0) - totdflux(0)
 
      do k = 1, nlay
        rfdelp(k) = heatfac / delp(k)
        fnet(k) = totuflux(k) - totdflux(k)
        htr(k) = (fnet(k-1) - fnet(k)) * rfdelp(k)
      enddo
 
!! --- ...  optional clear sky heating rates
      if ( lhlw0 ) then
        fnetc(0) = totuclfl(0) - totdclfl(0)
 
        do k = 1, nlay
          fnetc(k) = totuclfl(k) - totdclfl(k)
          htrcl(k) = (fnetc(k-1) - fnetc(k)) * rfdelp(k)
        enddo
      endif
 
!! --- ...  optional spectral band heating rates
      if ( lhlwb ) then
        do ib = 1, nbands
          fnet(0) = (toturad(0,ib) - totdrad(0,ib)) * flxfac
 
          do k = 1, nlay
            fnet(k) = (toturad(k,ib) - totdrad(k,ib)) * flxfac
            htrb(k,ib) = (fnet(k-1) - fnet(k)) * rfdelp(k)
          enddo
        enddo
      endif
 
! .................................
      end subroutine rtrnmr
! ---------------------------------
 
! ---------------------------------
      subroutine rtrnmc                                                 &
     &     ( semiss,delp,cldfmc,taucld,tautot,pklay,pklev,              & !  ---  inputs:
     &       fracs,secdif, nlay,nlp1,                                   &
     &       totuflux,totdflux,htr, totuclfl,totdclfl,htrcl, htrb       & !  ---  outputs:
     &     )
 
!  ===================  program usage description  ===================  !
!                                                                       !
! purpose:  compute the upward/downward radiative fluxes, and heating   !
! rates for both clear or cloudy atmosphere.  clouds are treated with   !
! the mcica stochastic approach.                                        !
!                                                                       !
! subprograms called:  none                                             !
!                                                                       !
!  ====================  defination of variables  ====================  !
!                                                                       !
!  inputs:                                                     -size-   !
!   semiss  - real, lw surface emissivity                         nbands!
!   delp    - real, layer pressure thickness (mb)                  nlay !
!   cldfmc  - real, layer cloud fraction (sub-column)        ngptlw*nlay!
!   taucld  - real, layer cloud opt depth                    nbands*nlay!
!   tautot  - real, total optical depth (gas+aerosols)       ngptlw*nlay!
!   pklay   - real, integrated planck func at lay temp     nbands*0:nlay!
!   pklev   - real, integrated planck func at lev temp     nbands*0:nlay!
!   fracs   - real, planck fractions                         ngptlw*nlay!
!   secdif  - real, secant of diffusivity angle                   nbands!
!   nlay    - integer, number of vertical layers                    1   !
!   nlp1    - integer, number of vertical levels (interfaces)       1   !
!                                                                       !
!  outputs:                                                             !
!   totuflux- real, total sky upward flux (w/m2)                 0:nlay !
!   totdflux- real, total sky downward flux (w/m2)               0:nlay !
!   htr     - real, total sky heating rate (k/sec or k/day)        nlay !
!   totuclfl- real, clear sky upward flux (w/m2)                 0:nlay !
!   totdclfl- real, clear sky downward flux (w/m2)               0:nlay !
!   htrcl   - real, clear sky heating rate (k/sec or k/day)        nlay !
!   htrb    - real, spectral band lw heating rate (k/day)    nlay*nbands!
!                                                                       !
!  module veriables:                                                    !
!   ngb     - integer, band index for each g-value                ngptlw!
!   fluxfac - real, conversion factor for fluxes (pi*2.e4)           1  !
!   heatfac - real, conversion factor for heating rates (g/cp*1e-2)  1  !
!   tblint  - real, conversion factor for look-up tbl (float(ntbl)   1  !
!   bpade   - real, pade approx constant (1/0.278)                   1  !
!   wtdiff  - real, weight for radiance to flux conversion           1  !
!   ntbl    - integer, dimension of look-up tables                   1  !
!   tau_tbl - real, clr-sky opt dep lookup table                 0:ntbl !
!   exp_tbl - real, transmittance lookup table                   0:ntbl !
!   tfn_tbl - real, tau transition function                      0:ntbl !
!                                                                       !
!  local variables:                                                     !
!    itgas  - integer, index for gases contribution look-up table    1  !
!    ittot  - integer, index for gases plus clouds  look-up table    1  !
!    reflct - real, surface reflectance                              1  !
!    atrgas - real, gaseous absorptivity                             1  !
!    atrtot - real, gaseous and cloud absorptivity                   1  !
!    odcld  - real, cloud optical depth                              1  !
!    efclrfr- real, effective clear sky fraction (1-efcldfr)        nlay!
!    odepth - real, optical depth of gaseous only                    1  !
!    odtot  - real, optical depth of gas and cloud                   1  !
!    gasfac - real, gas-only pade factor, used for planck function   1  !
!    totfac - real, gas and cloud pade factor, used for planck fn    1  !
!    bbdgas - real, gas-only planck function for downward rt         1  !
!    bbugas - real, gas-only planck function for upward rt           1  !
!    bbdtot - real, gas and cloud planck function for downward rt    1  !
!    bbutot - real, gas and cloud planck function for upward rt      1  !
!    gassrcu- real, upwd source radiance due to gas                 nlay!
!    totsrcu- real, upwd source radiance due to gas+cld             nlay!
!    gassrcd- real, dnwd source radiance due to gas                  1  !
!    totsrcd- real, dnwd source radiance due to gas+cld              1  !
!    radtotu- real, spectrally summed total sky upwd radiance        1  !
!    radclru- real, spectrally summed clear sky upwd radiance        1  !
!    radtotd- real, spectrally summed total sky dnwd radiance        1  !
!    radclrd- real, spectrally summed clear sky dnwd radiance        1  !
!    toturad- real, total sky upward radiance by layer     0:nlay*nbands!
!    clrurad- real, clear sky upward radiance by layer     0:nlay*nbands!
!    totdrad- real, total sky downward radiance by layer   0:nlay*nbands!
!    clrdrad- real, clear sky downward radiance by layer   0:nlay*nbands!
!    fnet   - real, net longwave flux (w/m2)                     0:nlay !
!    fnetc  - real, clear sky net longwave flux (w/m2)           0:nlay !
!                                                                       !
!                                                                       !
!  *******************************************************************  !
!  original code description                                            !
!                                                                       !
!  original version:   e. j. mlawer, et al. rrtm_v3.0                   !
!  revision for gcms:  michael j. iacono; october, 2002                 !
!  revision for f90:   michael j. iacono; june, 2006                    !
!                                                                       !
!  this program calculates the upward fluxes, downward fluxes, and      !
!  heating rates for an arbitrary clear or cloudy atmosphere. the input !
!  to this program is the atmospheric profile, all Planck function      !
!  information, and the cloud fraction by layer.  a variable diffusivity!
!  angle (secdif) is used for the angle integration. bands 2-3 and 5-9  !
!  use a value for secdif that varies from 1.50 to 1.80 as a function   !
!  of the column water vapor, and other bands use a value of 1.66.  the !
!  gaussian weight appropriate to this angle (wtdiff=0.5) is applied    !
!  here.  note that use of the emissivity angle for the flux integration!
!  can cause errors of 1 to 4 W/m2 within cloudy layers.                !
!  clouds are treated with the mcica stochastic approach and            !
!  maximum-random cloud overlap.                                        !
!                                                                       !
!  *******************************************************************  !
!  ======================  end of description block  =================  !
 
!  ---  inputs:
      integer, intent(in) :: nlay, nlp1
 
      real (kind=kind_phys), dimension(nbands), intent(in) :: semiss,   &
     &       secdif
      real (kind=kind_phys), dimension(nlay),   intent(in) :: delp
 
      real (kind=kind_phys), dimension(nbands,nlay),intent(in):: taucld
      real (kind=kind_phys), dimension(ngptlw,nlay),intent(in):: fracs, &
     &       tautot, cldfmc
 
      real (kind=kind_phys), dimension(nbands,0:nlay), intent(in) ::    &
     &       pklev, pklay
 
!  ---  outputs:
      real (kind=kind_phys), dimension(nlay), intent(out) :: htr, htrcl
 
      real (kind=kind_phys), dimension(nlay,nbands),intent(out) :: htrb
 
      real (kind=kind_phys), dimension(0:nlay), intent(out) ::          &
     &       totuflux, totdflux, totuclfl, totdclfl
 
!  ---  locals:
      real (kind=kind_phys), parameter :: rec_6 = 0.166667
 
      real (kind=kind_phys), dimension(0:nlay,nbands) :: clrurad,       &
     &       clrdrad, toturad, totdrad
 
      real (kind=kind_phys), dimension(nlay)   :: gassrcu, totsrcu,     &
     &       trngas, efclrfr, rfdelp
      real (kind=kind_phys), dimension(0:nlay) :: fnet, fnetc
 
      real (kind=kind_phys) :: totsrcd, gassrcd, tblind, odepth, odtot, &
     &       odcld, atrtot, atrgas, reflct, totfac, gasfac, flxfac,     &
     &       plfrac, blay, bbdgas, bbdtot, bbugas, bbutot, dplnku,      &
     &       dplnkd, radtotu, radclru, radtotd, radclrd, rad0,          &
     &       clfm, trng, gasu
 
      integer :: ittot, itgas, ib, ig, k
!
!===> ...  begin here
!
      do ib = 1, nbands
        do k = 0, nlay
          toturad(k,ib) = f_zero
          totdrad(k,ib) = f_zero
          clrurad(k,ib) = f_zero
          clrdrad(k,ib) = f_zero
        enddo
      enddo
 
      do k = 0, nlay
        totuflux(k) = f_zero
        totdflux(k) = f_zero
        totuclfl(k) = f_zero
        totdclfl(k) = f_zero
      enddo
 
!  --- ...  loop over all g-points
 
      do ig = 1, ngptlw
        ib = ngb(ig)
 
        radtotd = f_zero
        radclrd = f_zero
 
 
        do k = nlay, 1, -1
 
!  --- ...  clear sky, gases contribution
 
          odepth = max( f_zero, secdif(ib)*tautot(ig,k) )
          if (odepth <= 0.06) then
            atrgas = odepth - 0.5*odepth*odepth
            trng   = f_one - atrgas
            gasfac = rec_6 * odepth
          else
            tblind = odepth / (bpade + odepth)
            itgas = tblint*tblind + 0.5
            trng  = exp_tbl(itgas)
            atrgas = f_one - trng
            gasfac = tfn_tbl(itgas)
            odepth = tau_tbl(itgas)
          endif
 
          plfrac = fracs(ig,k)
          blay = pklay(ib,k)
 
          dplnku = pklev(ib,k  ) - blay
          dplnkd = pklev(ib,k-1) - blay
          bbdgas = plfrac * (blay + dplnkd*gasfac)
          bbugas = plfrac * (blay + dplnku*gasfac)
          gassrcd= bbdgas * atrgas
          gassrcu(k)= bbugas * atrgas
          trngas(k) = trng
 
!  --- ...  total sky, gases+clouds contribution
 
          clfm = cldfmc(ig,k)
          if (clfm >= eps) then
!  --- ...  cloudy layer
 
            odcld = secdif(ib) * taucld(ib,k)
            efclrfr(k) = f_one - (f_one - exp(-odcld))*clfm
            odtot = odepth + odcld
            if (odtot < 0.06) then
              totfac = rec_6 * odtot
              atrtot = odtot - 0.5*odtot*odtot
            else
              tblind = odtot / (bpade + odtot)
              ittot  = tblint*tblind + 0.5
              totfac = tfn_tbl(ittot)
              atrtot = f_one - exp_tbl(ittot)
            endif
 
            bbdtot = plfrac * (blay + dplnkd*totfac)
            bbutot = plfrac * (blay + dplnku*totfac)
            totsrcd= bbdtot * atrtot
            totsrcu(k)= bbutot * atrtot
 
!  --- ...  total sky radiance
            radtotd = radtotd*trng*efclrfr(k) + gassrcd                 &
     &              + clfm*(totsrcd - gassrcd)
            totdrad(k-1,ib) = totdrad(k-1,ib) + radtotd
 
!  --- ...  clear sky radiance
            radclrd = radclrd*trng + gassrcd
            clrdrad(k-1,ib) = clrdrad(k-1,ib) + radclrd
 
          else
!  --- ...  clear layer
 
!  --- ...  total sky radiance
            radtotd = radtotd*trng + gassrcd
            totdrad(k-1,ib) = totdrad(k-1,ib) + radtotd
 
!  --- ...  clear sky radiance
            radclrd = radclrd*trng + gassrcd
            clrdrad(k-1,ib) = clrdrad(k-1,ib) + radclrd
 
          endif   ! end if_clfm_block
 
        enddo   ! end do_k_loop
 
 
!     note: spectral and Lambertian reflection are identical for the
!           diffusivity angle flux integration used here.
 
        reflct = f_one - semiss(ib)
        rad0 = semiss(ib) * fracs(ig,1) * pklay(ib,0)
 
        radtotu = rad0 + reflct*radtotd
        toturad(0,ib) = toturad(0,ib) + radtotu
 
        radclru = rad0 + reflct*radclrd
        clrurad(0,ib) = clrurad(0,ib) + radclru
 
 
!          toturad holds summed radiance for total sky stream
!          clrurad holds summed radiance for clear sky stream
 
        do k = 1, nlay
          clfm = cldfmc(ig,k)
          trng = trngas(k)
          gasu = gassrcu(k)
 
          if (clfm > eps) then
!  --- ...  cloudy layer
 
!  --- ... total sky radiance
            radtotu = radtotu*trng*efclrfr(k) + gasu                    &
     &              + clfm*(totsrcu(k) - gasu)
            toturad(k,ib) = toturad(k,ib) + radtotu
 
!  --- ... clear sky radiance
            radclru = radclru*trng + gasu
            clrurad(k,ib) = clrurad(k,ib) + radclru
 
          else
!  --- ...  clear layer
 
!  --- ... total sky radiance
            radtotu = radtotu*trng + gasu
            toturad(k,ib) = toturad(k,ib) + radtotu
 
!  --- ... clear sky radiance
            radclru = radclru*trng + gasu
            clrurad(k,ib) = clrurad(k,ib) + radclru
 
          endif   ! end if_clfm_block
 
        enddo   ! end do_k_loop
 
      enddo   ! end do_ig_loop
 
 
      flxfac = wtdiff * fluxfac
 
      do k = 0, nlay
        do ib = 1, nbands
          totuflux(k) = totuflux(k) + toturad(k,ib)
          totdflux(k) = totdflux(k) + totdrad(k,ib)
          totuclfl(k) = totuclfl(k) + clrurad(k,ib)
          totdclfl(k) = totdclfl(k) + clrdrad(k,ib)
        enddo
 
        totuflux(k) = totuflux(k) * flxfac
        totdflux(k) = totdflux(k) * flxfac
        totuclfl(k) = totuclfl(k) * flxfac
        totdclfl(k) = totdclfl(k) * flxfac
      enddo
 
      fnet(0) = totuflux(0) - totdflux(0)
 
      do k = 1, nlay
        rfdelp(k) = heatfac / delp(k)
        fnet(k) = totuflux(k) - totdflux(k)
        htr(k) = (fnet(k-1) - fnet(k)) * rfdelp(k)
      enddo
 
      if ( lhlw0 ) then
        fnetc(0) = totuclfl(0) - totdclfl(0)
 
        do k = 1, nlay
          fnetc(k) = totuclfl(k) - totdclfl(k)
          htrcl(k) = (fnetc(k-1) - fnetc(k)) * rfdelp(k)
        enddo
      endif
 
      if ( lhlwb ) then
        do ib = 1, nbands
          fnet(0) = (toturad(0,ib) - totdrad(0,ib)) * flxfac
 
          do k = 1, nlay
            fnet(k) = (toturad(k,ib) - totdrad(k,ib)) * flxfac
            htrb(k,ib) = (fnet(k-1) - fnet(k)) * rfdelp(k)
          enddo
        enddo
      endif
 
! ..................................
      end subroutine rtrnmc
! ----------------------------------
 
      subroutine taumol                                                 &
     &     ( laytrop,pavel,coldry,colamt,colbrd,wx,tauaer,              & !  ---  inputs
     &       rfrate,fac00,fac01,fac10,fac11,jp,jt,jt1,                  &
     &       selffac,selffrac,indself,forfac,forfrac,indfor,            &
     &       minorfrac,scaleminor,scaleminorn2,indminor,                &
     &       nlay,                                                      &
     &       fracs, tautot                                              & !  ---  outputs
     &     )
 
!  ************    original subprogram description    ***************   !
!                                                                       !
!                  optical depths developed for the                     !
!                                                                       !
!                rapid radiative transfer model (rrtm)                  !
!                                                                       !
!            atmospheric and environmental research, inc.               !
!                        131 hartwell avenue                            !
!                        lexington, ma 02421                            !
!                                                                       !
!                           eli j. mlawer                               !
!                         jennifer delamere                             !
!                         steven j. taubman                             !
!                         shepard a. clough                             !
!                                                                       !
!                       email:  mlawer@aer.com                          !
!                       email:  jdelamer@aer.com                        !
!                                                                       !
!        the authors wish to acknowledge the contributions of the       !
!        following people:  karen cady-pereira, patrick d. brown,       !
!        michael j. iacono, ronald e. farren, luke chen,                !
!        robert bergstrom.                                              !
!                                                                       !
!  revision for g-point reduction: michael j. iacono; aer, inc.         !
!                                                                       !
!     taumol                                                            !
!                                                                       !
!     this file contains the subroutines taugbn (where n goes from      !
!     1 to 16).  taugbn calculates the optical depths and planck        !
!     fractions per g-value and layer for band n.                       !
!                                                                       !
!  *******************************************************************  !
!  ==================   program usage description   ==================  !
!                                                                       !
!    call  taumol                                                       !
!       inputs:                                                         !
!          ( laytrop,pavel,coldry,colamt,colbrd,wx,tauaer,              !
!            rfrate,fac00,fac01,fac10,fac11,jp,jt,jt1,                  !
!            selffac,selffrac,indself,forfac,forfrac,indfor,            !
!            minorfrac,scaleminor,scaleminorn2,indminor,                !
!            nlay,                                                      !
!       outputs:                                                        !
!            fracs, tautot )                                            !
!                                                                       !
!  subprograms called:  taugb## (## = 01 -16)                           !
!                                                                       !
!                                                                       !
!  ====================  defination of variables  ====================  !
!                                                                       !
!  inputs:                                                        size  !
!     laytrop   - integer, tropopause layer index (unitless)        1   !
!                   layer at which switch is made for key species       !
!     pavel     - real, layer pressures (mb)                       nlay !
!     coldry    - real, column amount for dry air (mol/cm2)        nlay !
!     colamt    - real, column amounts of h2o, co2, o3, n2o, ch4,       !
!                   o2, co (mol/cm**2)                       nlay*maxgas!
!     colbrd    - real, column amount of broadening gases          nlay !
!     wx        - real, cross-section amounts(mol/cm2)      nlay*maxxsec!
!     tauaer    - real, aerosol optical depth               nbands*nlay !
!     rfrate    - real, reference ratios of binary species parameter    !
!     (:,m,:)m=1-h2o/co2,2-h2o/o3,3-h2o/n2o,4-h2o/ch4,5-n2o/co2,6-o3/co2!
!     (:,:,n)n=1,2: the rates of ref press at the 2 sides of the layer  !
!                                                          nlay*nrates*2!
!     facij     - real, factors multiply the reference ks, i,j of 0/1   !
!                   for lower/higher of the 2 appropriate temperatures  !
!                   and altitudes                                  nlay !
!     jp        - real, index of lower reference pressure          nlay !
!     jt, jt1   - real, indices of lower reference temperatures    nlay !
!                   for pressure levels jp and jp+1, respectively       !
!     selffac   - real, scale factor for water vapor self-continuum     !
!                   equals (water vapor density)/(atmospheric density   !
!                   at 296k and 1013 mb)                           nlay !
!     selffrac  - real, factor for temperature interpolation of         !
!                   reference water vapor self-continuum data      nlay !
!     indself   - integer, index of lower reference temperature for     !
!                   the self-continuum interpolation               nlay !
!     forfac    - real, scale factor for w. v. foreign-continuum   nlay !
!     forfrac   - real, factor for temperature interpolation of         !
!                   reference w.v. foreign-continuum data          nlay !
!     indfor    - integer, index of lower reference temperature for     !
!                   the foreign-continuum interpolation            nlay !
!     minorfrac - real, factor for minor gases                     nlay !
!     scaleminor,scaleminorn2                                           !
!               - real, scale factors for minor gases              nlay !
!     indminor  - integer, index of lower reference temperature for     !
!                   minor gases                                    nlay !
!     nlay      - integer, total number of layers                   1   !
!                                                                       !
!  outputs:                                                             !
!     fracs     - real, planck fractions                     ngptlw,nlay!
!     tautot    - real, total optical depth (gas+aerosols)   ngptlw,nlay!
!                                                                       !
!  internal variables:                                                  !
!     ng##      - integer, number of g-values in band ## (##=01-16) 1   !
!     nspa      - integer, for lower atmosphere, the number of ref      !
!                   atmos, each has different relative amounts of the   !
!                   key species for the band                      nbands!
!     nspb      - integer, same but for upper atmosphere          nbands!
!     absa      - real, k-values for lower ref atmospheres (no w.v.     !
!                   self-continuum) (cm**2/molecule)  nspa(##)*5*13*ng##!
!     absb      - real, k-values for high ref atmospheres (all sources) !
!                   (cm**2/molecule)               nspb(##)*5*13:59*ng##!
!     ka_m'mgas'- real, k-values for low ref atmospheres minor species  !
!                   (cm**2/molecule)                          mmn##*ng##!
!     kb_m'mgas'- real, k-values for high ref atmospheres minor species !
!                   (cm**2/molecule)                          mmn##*ng##!
!     selfref   - real, k-values for w.v. self-continuum for ref atmos  !
!                   used below laytrop (cm**2/mol)               10*ng##!
!     forref    - real, k-values for w.v. foreign-continuum for ref atmos
!                   used below/above laytrop (cm**2/mol)          4*ng##!
!                                                                       !
!  ******************************************************************   !
 
!  ---  inputs:
      integer, intent(in) :: nlay, laytrop
 
      integer, dimension(nlay), intent(in) :: jp, jt, jt1, indself,     &
     &       indfor, indminor
 
      real (kind=kind_phys), dimension(nlay), intent(in) :: pavel,      &
     &       coldry, colbrd, fac00, fac01, fac10, fac11, selffac,       &
     &       selffrac, forfac, forfrac, minorfrac, scaleminor,          &
     &       scaleminorn2
 
      real (kind=kind_phys), dimension(nlay,maxgas), intent(in):: colamt
      real (kind=kind_phys), dimension(nlay,maxxsec),intent(in):: wx
 
      real (kind=kind_phys), dimension(nbands,nlay), intent(in):: tauaer
 
      real (kind=kind_phys), dimension(nlay,nrates,2), intent(in) ::    &
     &       rfrate
 
!  ---  outputs:
      real (kind=kind_phys), dimension(ngptlw,nlay), intent(out) ::     &
     &       fracs, tautot
 
!  ---  locals
      real (kind=kind_phys), dimension(ngptlw,nlay) :: taug
 
      integer :: ib, ig, k
!
!===> ...  begin here
!
      call taugb01
      call taugb02
      call taugb03
      call taugb04
      call taugb05
      call taugb06
      call taugb07
      call taugb08
      call taugb09
      call taugb10
      call taugb11
      call taugb12
      call taugb13
      call taugb14
      call taugb15
      call taugb16
 
!  ---  combine gaseous and aerosol optical depths
 
      do ig = 1, ngptlw
        ib = ngb(ig)
 
        do k = 1, nlay
          tautot(ig,k) = taug(ig,k) + tauaer(ib,k)
        enddo
      enddo
 
! =================
      contains
! =================
 
! ----------------------------------
      subroutine taugb01
! ..................................
 
!  ------------------------------------------------------------------  !
!  written by eli j. mlawer, atmospheric & environmental research.     !
!  revised by michael j. iacono, atmospheric & environmental research. !
!                                                                      !
!     band 1:  10-350 cm-1 (low key - h2o; low minor - n2)             !
!                          (high key - h2o; high minor - n2)           !
!                                                                      !
!  compute the optical depth by interpolating in ln(pressure) and      !
!  temperature.  below laytrop, the water vapor self-continuum and     !
!  foreign continuum is interpolated (in temperature) separately.      !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb01
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &           indm, indmp, ig
 
      real (kind=kind_phys) :: pp, corradj, scalen2, tauself, taufor,   &
     &       taun2
!
!===> ...  begin here
!
!  ---  minor gas mapping levels:
!     lower - n2, p = 142.5490 mbar, t = 215.70 k
!     upper - n2, p = 142.5490 mbar, t = 215.70 k
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(1) + 1
        ind1 = ( jp(k)   *5 + (jt1(k)-1)) * nspa(1) + 1
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
 
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
 
        pp = pavel(k)
        scalen2 = colbrd(k) * scaleminorn2(k)
        if (pp < 250.0) then
          corradj = f_one - 0.15 * (250.0-pp) / 154.4
        else
          corradj = f_one
        endif
 
        do ig = 1, ng01
          tauself = selffac(k) * (selfref(ig,inds) + selffrac(k)        &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) -  forref(ig,indf)))
          taun2   = scalen2 * (ka_mn2(ig,indm) + minorfrac(k)           &
     &            * (ka_mn2(ig,indmp) - ka_mn2(ig,indm)))
 
          taug(ig,k) = corradj * (colamt(k,1)                           &
     &            * (fac00(k)*absa(ig,ind0) + fac10(k)*absa(ig,ind0p)   &
     &            +  fac01(k)*absa(ig,ind1) + fac11(k)*absa(ig,ind1p))  &
     &            + tauself + taufor + taun2)
 
          fracs(ig,k) = fracrefa(ig)
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(1) + 1
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(1) + 1
        indf = indfor(k)
        indm = indminor(k)
 
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indfp = indf + 1
        indmp = indm + 1
 
        scalen2 = colbrd(k) * scaleminorn2(k)
        corradj = f_one - 0.15 * (pavel(k) / 95.6)
 
        do ig = 1, ng01
          taufor = forfac(k) * (forref(ig,indf) + forfrac(k)            &
     &           * (forref(ig,indfp) - forref(ig,indf)))
          taun2  = scalen2 * (kb_mn2(ig,indm) + minorfrac(k)            &
     &           * (kb_mn2(ig,indmp) - kb_mn2(ig,indm)))
 
          taug(ig,k) = corradj * (colamt(k,1)                           &
     &           * (fac00(k)*absb(ig,ind0) + fac10(k)*absb(ig,ind0p)    &
     &           +  fac01(k)*absb(ig,ind1) + fac11(k)*absb(ig,ind1p))   &
     &           + taufor + taun2)
 
          fracs(ig,k) = fracrefb(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb01
! ----------------------------------
 
! ----------------------------------
      subroutine taugb02
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 2:  350-500 cm-1 (low key - h2o; high key - h2o)            !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb02
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &           ig
 
      real (kind=kind_phys) :: corradj, tauself, taufor
!
!===> ...  begin here
!
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(2) + 1
        ind1 = ( jp(k)   *5 + (jt1(k)-1)) * nspa(2) + 1
        inds = indself(k)
        indf = indfor(k)
 
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indsp = inds + 1
        indfp = indf + 1
 
        corradj = f_one - 0.05 * (pavel(k) - 100.0) / 900.0
 
        do ig = 1, ng02
          tauself = selffac(k) * (selfref(ig,inds) + selffrac(k)        &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
 
          taug(ns02+ig,k) = corradj * (colamt(k,1)                      &
     &            * (fac00(k)*absa(ig,ind0) + fac10(k)*absa(ig,ind0p)   &
     &            +  fac01(k)*absa(ig,ind1) + fac11(k)*absa(ig,ind1p))  &
     &            + tauself + taufor)
 
          fracs(ns02+ig,k) = fracrefa(ig)
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(2) + 1
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(2) + 1
        indf = indfor(k)
 
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indfp = indf + 1
 
        do ig = 1, ng02
          taufor = forfac(k) * (forref(ig,indf) + forfrac(k)            &
     &           * (forref(ig,indfp) - forref(ig,indf)))
 
          taug(ns02+ig,k) = colamt(k,1)                                 &
     &           * (fac00(k)*absb(ig,ind0) + fac10(k)*absb(ig,ind0p)    &
     &           +  fac01(k)*absb(ig,ind1) + fac11(k)*absb(ig,ind1p))   &
     &           + taufor
 
          fracs(ns02+ig,k) = fracrefb(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb02
! ----------------------------------
 
! ----------------------------------
      subroutine taugb03
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 3:  500-630 cm-1 (low key - h2o,co2; low minor - n2o)       !
!                           (high key - h2o,co2; high minor - n2o)     !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb03
 
!  ---  locals:
      integer :: k, ind0, ind1, inds, indsp, indf, indfp, indm, indmp,  &
     &       id000, id010, id100, id110, id200, id210, jmn2o, jmn2op,   &
     &       id001, id011, id101, id111, id201, id211, jpl, jplp,       &
     &       ig, js, js1
 
      real (kind=kind_phys) ::  absn2o, ratn2o, adjfac, adjcoln2o,      &
     &      speccomb,       specparm,       specmult,       fs,         &
     &      speccomb1,      specparm1,      specmult1,      fs1,        &
     &      speccomb_mn2o,  specparm_mn2o,  specmult_mn2o,  fmn2o,      &
     &      speccomb_planck,specparm_planck,specmult_planck,fpl,        &
     &      refrat_planck_a, refrat_planck_b, refrat_m_a, refrat_m_b,   &
     &      fac000, fac100, fac200, fac010, fac110, fac210,             &
     &      fac001, fac101, fac201, fac011, fac111, fac211,             &
     &      tau_major, tau_major1, tauself, taufor, n2om1, n2om2,       &
     &      p, p4, fk0, fk1, fk2
!
!===> ...  begin here
!
!  --- ...  minor gas mapping levels:
!     lower - n2o, p = 706.272 mbar, t = 278.94 k
!     upper - n2o, p = 95.58 mbar, t = 215.7 k
 
      refrat_planck_a = chi_mls(1,9)/chi_mls(2,9)    ! P = 212.725 mb
      refrat_planck_b = chi_mls(1,13)/chi_mls(2,13)  ! P = 95.58   mb
      refrat_m_a      = chi_mls(1,3)/chi_mls(2,3)    ! P = 706.270 mb
      refrat_m_b      = chi_mls(1,13)/chi_mls(2,13)  ! P = 95.58   mb
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        speccomb = colamt(k,1) + rfrate(k,1,1)*colamt(k,2)
        specparm = colamt(k,1) / speccomb
        specmult = 8.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(3) + js
 
        speccomb1 = colamt(k,1) + rfrate(k,1,2)*colamt(k,2)
        specparm1 = colamt(k,1) / speccomb1
        specmult1 = 8.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = (jp(k)*5 + (jt1(k)-1)) * nspa(3) + js1
 
        speccomb_mn2o = colamt(k,1) + refrat_m_a*colamt(k,2)
        specparm_mn2o = colamt(k,1) / speccomb_mn2o
        specmult_mn2o = 8.0 * min(specparm_mn2o, oneminus)
        jmn2o = 1 + int(specmult_mn2o)
        fmn2o = mod(specmult_mn2o, f_one)
 
        speccomb_planck = colamt(k,1) + refrat_planck_a*colamt(k,2)
        specparm_planck = colamt(k,1) / speccomb_planck
        specmult_planck = 8.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
 
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
        jmn2op= jmn2o+ 1
        jplp  = jpl  + 1
 
!  --- ...  in atmospheres where the amount of n2O is too great to be considered
!           a minor species, adjust the column amount of n2O by an empirical factor
!           to obtain the proper contribution.
 
        p = coldry(k) * chi_mls(4,jp(k)+1)
        ratn2o = colamt(k,4) / p
        if (ratn2o > 1.5) then
          adjfac = 0.5 + (ratn2o - 0.5)**0.65
          adjcoln2o = adjfac * p
        else
          adjcoln2o = colamt(k,4)
        endif
 
        if (specparm < 0.125) then
          p = fs - f_one
          p4 = p**4
          fk0 = p4
          fk1 = f_one - p - 2.0*p4
          fk2 = p + p4
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0 + 2
          id210 = ind0 +11
        else if (specparm > 0.875) then
          p = -fs
          p4 = p**4
          fk0 = p4
          fk1 = f_one - p - 2.0*p4
          fk2 = p + p4
          id000 = ind0 + 1
          id010 = ind0 +10
          id100 = ind0
          id110 = ind0 + 9
          id200 = ind0 - 1
          id210 = ind0 + 8
        else
          fk0 = f_one - fs
          fk1 = fs
          fk2 = f_zero
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0
          id210 = ind0
        endif
 
        fac000 = fk0*fac00(k)
        fac100 = fk1*fac00(k)
        fac200 = fk2*fac00(k)
        fac010 = fk0*fac10(k)
        fac110 = fk1*fac10(k)
        fac210 = fk2*fac10(k)
 
        if (specparm1 < 0.125) then
          p = fs1 - f_one
          p4 = p**4
          fk0 = p4
          fk1 = f_one - p - 2.0*p4
          fk2 = p + p4
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1 + 2
          id211 = ind1 +11
        elseif (specparm1 > 0.875) then
          p = -fs1
          p4 = p**4
          fk0 = p4
          fk1 = f_one - p - 2.0*p4
          fk2 = p + p4
          id001 = ind1 + 1
          id011 = ind1 +10
          id101 = ind1
          id111 = ind1 + 9
          id201 = ind1 - 1
          id211 = ind1 + 8
        else
          fk0 = f_one - fs1
          fk1 = fs1
          fk2 = f_zero
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1
          id211 = ind1
        endif
 
        fac001 = fk0*fac01(k)
        fac101 = fk1*fac01(k)
        fac201 = fk2*fac01(k)
        fac011 = fk0*fac11(k)
        fac111 = fk1*fac11(k)
        fac211 = fk2*fac11(k)
 
        do ig = 1, ng03
          tauself = selffac(k)* (selfref(ig,inds) + selffrac(k)         &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
          n2om1   = ka_mn2o(ig,jmn2o,indm) + fmn2o                      &
     &            * (ka_mn2o(ig,jmn2op,indm) - ka_mn2o(ig,jmn2o,indm))
          n2om2   = ka_mn2o(ig,jmn2o,indmp) + fmn2o                     &
     &            * (ka_mn2o(ig,jmn2op,indmp) - ka_mn2o(ig,jmn2o,indmp))
          absn2o  = n2om1 + minorfrac(k) * (n2om2 - n2om1)
 
          tau_major = speccomb                                          &
     &              * (fac000*absa(ig,id000) + fac010*absa(ig,id010)    &
     &              +  fac100*absa(ig,id100) + fac110*absa(ig,id110)    &
     &              +  fac200*absa(ig,id200) + fac210*absa(ig,id210))
 
          tau_major1 = speccomb1                                        &
     &              * (fac001*absa(ig,id001) + fac011*absa(ig,id011)    &
     &              +  fac101*absa(ig,id101) + fac111*absa(ig,id111)    &
     &              +  fac201*absa(ig,id201) + fac211*absa(ig,id211))
 
          taug(ns03+ig,k) = tau_major + tau_major1                      &
     &                    + tauself + taufor + adjcoln2o*absn2o
 
          fracs(ns03+ig,k) = fracrefa(ig,jpl) + fpl                     &
     &                     * (fracrefa(ig,jplp) - fracrefa(ig,jpl))
        enddo     ! end do_k_loop
      enddo   ! end do_ig_loop
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        speccomb = colamt(k,1) + rfrate(k,1,1)*colamt(k,2)
        specparm = colamt(k,1) / speccomb
        specmult = 4.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(3) + js
 
        speccomb1 = colamt(k,1) + rfrate(k,1,2)*colamt(k,2)
        specparm1 = colamt(k,1) / speccomb1
        specmult1 = 4.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(3) + js1
 
        speccomb_mn2o = colamt(k,1) + refrat_m_b*colamt(k,2)
        specparm_mn2o = colamt(k,1) / speccomb_mn2o
        specmult_mn2o = 4.0 * min(specparm_mn2o, oneminus)
        jmn2o = 1 + int(specmult_mn2o)
        fmn2o = mod(specmult_mn2o, f_one)
 
        speccomb_planck = colamt(k,1) + refrat_planck_b*colamt(k,2)
        specparm_planck = colamt(k,1) / speccomb_planck
        specmult_planck = 4.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
 
        indf = indfor(k)
        indm = indminor(k)
        indfp = indf + 1
        indmp = indm + 1
        jmn2op= jmn2o+ 1
        jplp  = jpl  + 1
 
        id000 = ind0
        id010 = ind0 + 5
        id100 = ind0 + 1
        id110 = ind0 + 6
        id001 = ind1
        id011 = ind1 + 5
        id101 = ind1 + 1
        id111 = ind1 + 6
 
!  --- ...  in atmospheres where the amount of n2o is too great to be considered
!           a minor species, adjust the column amount of N2O by an empirical factor
!           to obtain the proper contribution.
 
        p = coldry(k) * chi_mls(4,jp(k)+1)
        ratn2o = colamt(k,4) / p
        if (ratn2o > 1.5) then
          adjfac = 0.5 + (ratn2o - 0.5)**0.65
          adjcoln2o = adjfac * p
        else
          adjcoln2o = colamt(k,4)
        endif
 
        fk0 = f_one - fs
        fk1 = fs
        fac000 = fk0*fac00(k)
        fac010 = fk0*fac10(k)
        fac100 = fk1*fac00(k)
        fac110 = fk1*fac10(k)
 
        fk0 = f_one - fs1
        fk1 = fs1
        fac001 = fk0*fac01(k)
        fac011 = fk0*fac11(k)
        fac101 = fk1*fac01(k)
        fac111 = fk1*fac11(k)
 
        do ig = 1, ng03
          taufor = forfac(k) * (forref(ig,indf) + forfrac(k)            &
     &           * (forref(ig,indfp) - forref(ig,indf)))
          n2om1  = kb_mn2o(ig,jmn2o,indm) + fmn2o                       &
     &           * (kb_mn2o(ig,jmn2op,indm) - kb_mn2o(ig,jmn2o,indm))
          n2om2  = kb_mn2o(ig,jmn2o,indmp) + fmn2o                      &
     &           * (kb_mn2o(ig,jmn2op,indmp) - kb_mn2o(ig,jmn2o,indmp))
          absn2o = n2om1 + minorfrac(k) * (n2om2 - n2om1)
 
          tau_major = speccomb                                          &
     &              * (fac000*absb(ig,id000) + fac010*absb(ig,id010)    &
     &              +  fac100*absb(ig,id100) + fac110*absb(ig,id110))
 
          tau_major1 = speccomb1                                        &
     &              * (fac001*absb(ig,id001) + fac011*absb(ig,id011)    &
     &              +  fac101*absb(ig,id101) + fac111*absb(ig,id111))
 
          taug(ns03+ig,k) = tau_major + tau_major1                      &
     &                    + taufor + adjcoln2o*absn2o
 
          fracs(ns03+ig,k) = fracrefb(ig,jpl) + fpl                     &
     &                     * (fracrefb(ig,jplp) - fracrefb(ig,jpl))
        enddo
      enddo
 
! ..................................
      end subroutine taugb03
! ----------------------------------
 
! ----------------------------------
      subroutine taugb04
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 4:  630-700 cm-1 (low key - h2o,co2; high key - o3,co2)     !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb04
 
!  ---  locals:
      integer :: k, ind0, ind1, inds, indsp, indf, indfp, jpl, jplp,    &
     &       id000, id010, id100, id110, id200, id210, ig, js, js1,     &
     &       id001, id011, id101, id111, id201, id211
 
      real (kind=kind_phys) :: tauself, taufor, p, p4, fk0, fk1, fk2,   &
     &      speccomb,       specparm,       specmult,       fs,         &
     &      speccomb1,      specparm1,      specmult1,      fs1,        &
     &      speccomb_planck,specparm_planck,specmult_planck,fpl,        &
     &      fac000, fac100, fac200, fac010, fac110, fac210,             &
     &      fac001, fac101, fac201, fac011, fac111, fac211,             &
     &      refrat_planck_a, refrat_planck_b, tau_major, tau_major1
!
!===> ...  begin here
!
      refrat_planck_a = chi_mls(1,11)/chi_mls(2,11)     ! P = 142.5940 mb
      refrat_planck_b = chi_mls(3,13)/chi_mls(2,13)     ! P = 95.58350 mb
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        speccomb = colamt(k,1) + rfrate(k,1,1)*colamt(k,2)
        specparm = colamt(k,1) / speccomb
        specmult = 8.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(4) + js
 
        speccomb1 = colamt(k,1) + rfrate(k,1,2)*colamt(k,2)
        specparm1 = colamt(k,1) / speccomb1
        specmult1 = 8.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = ( jp(k)*5 + (jt1(k)-1)) * nspa(4) + js1
 
        speccomb_planck = colamt(k,1) + refrat_planck_a*colamt(k,2)
        specparm_planck = colamt(k,1) / speccomb_planck
        specmult_planck = 8.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, 1.0)
 
        inds = indself(k)
        indf = indfor(k)
        indsp = inds + 1
        indfp = indf + 1
        jplp  = jpl  + 1
 
        if (specparm < 0.125) then
          p = fs - f_one
          p4 = p**4
          fk0 = p4
          fk1 = f_one - p - 2.0*p4
          fk2 = p + p4
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0 + 2
          id210 = ind0 +11
        elseif (specparm > 0.875) then
          p = -fs
          p4 = p**4
          fk0 = p4
          fk1 = f_one - p - 2.0*p4
          fk2 = p + p4
          id000 = ind0 + 1
          id010 = ind0 +10
          id100 = ind0
          id110 = ind0 + 9
          id200 = ind0 - 1
          id210 = ind0 + 8
        else
          fk0 = f_one - fs
          fk1 = fs
          fk2 = f_zero
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0
          id210 = ind0
        endif
 
        fac000 = fk0*fac00(k)
        fac100 = fk1*fac00(k)
        fac200 = fk2*fac00(k)
        fac010 = fk0*fac10(k)
        fac110 = fk1*fac10(k)
        fac210 = fk2*fac10(k)
 
        if (specparm1 < 0.125) then
          p = fs1 - f_one
          p4 = p**4
          fk0 = p4
          fk1 = f_one - p - 2.0*p4
          fk2 = p + p4
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1 + 2
          id211 = ind1 +11
        elseif (specparm1 > 0.875) then
          p = -fs1
          p4 = p**4
          fk0 = p4
          fk1 = f_one - p - 2.0*p4
          fk2 = p + p4
          id001 = ind1 + 1
          id011 = ind1 +10
          id101 = ind1
          id111 = ind1 + 9
          id201 = ind1 - 1
          id211 = ind1 + 8
        else
          fk0 = f_one - fs1
          fk1 = fs1
          fk2 = f_zero
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1
          id211 = ind1
        endif
 
        fac001 = fk0*fac01(k)
        fac101 = fk1*fac01(k)
        fac201 = fk2*fac01(k)
        fac011 = fk0*fac11(k)
        fac111 = fk1*fac11(k)
        fac211 = fk2*fac11(k)
 
        do ig = 1, ng04
          tauself = selffac(k)* (selfref(ig,inds) + selffrac(k)         &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
 
          tau_major = speccomb                                          &
     &              * (fac000*absa(ig,id000) + fac010*absa(ig,id010)    &
     &              +  fac100*absa(ig,id100) + fac110*absa(ig,id110)    &
     &              +  fac200*absa(ig,id200) + fac210*absa(ig,id210))
 
          tau_major1 = speccomb1                                        &
     &              * (fac001*absa(ig,id001) + fac011*absa(ig,id011)    &
     &              +  fac101*absa(ig,id101) + fac111*absa(ig,id111)    &
     &              +  fac201*absa(ig,id201) + fac211*absa(ig,id211))
 
          taug(ns04+ig,k) = tau_major + tau_major1 + tauself + taufor
 
          fracs(ns04+ig,k) = fracrefa(ig,jpl) + fpl                     &
     &                     * (fracrefa(ig,jplp) - fracrefa(ig,jpl))
        enddo     ! end do_k_loop
      enddo   ! end do_ig_loop
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        speccomb = colamt(k,3) + rfrate(k,6,1)*colamt(k,2)
        specparm = colamt(k,3) / speccomb
        specmult = 4.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(4) + js
 
        speccomb1 = colamt(k,3) + rfrate(k,6,2)*colamt(k,2)
        specparm1 = colamt(k,3) / speccomb1
        specmult1 = 4.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(4) + js1
 
        speccomb_planck = colamt(k,3) + refrat_planck_b*colamt(k,2)
        specparm_planck = colamt(k,3) / speccomb_planck
        specmult_planck = 4.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
        jplp = jpl + 1
 
        id000 = ind0
        id010 = ind0 + 5
        id100 = ind0 + 1
        id110 = ind0 + 6
        id001 = ind1
        id011 = ind1 + 5
        id101 = ind1 + 1
        id111 = ind1 + 6
 
        fk0 = f_one - fs
        fk1 = fs
        fac000 = fk0*fac00(k)
        fac010 = fk0*fac10(k)
        fac100 = fk1*fac00(k)
        fac110 = fk1*fac10(k)
 
        fk0 = f_one - fs1
        fk1 = fs1
        fac001 = fk0*fac01(k)
        fac011 = fk0*fac11(k)
        fac101 = fk1*fac01(k)
        fac111 = fk1*fac11(k)
 
        do ig = 1, ng04
          tau_major =  speccomb                                         &
     &              * (fac000*absb(ig,id000) + fac010*absb(ig,id010)    &
     &              +  fac100*absb(ig,id100) + fac110*absb(ig,id110))
          tau_major1 = speccomb1                                        &
     &              * (fac001*absb(ig,id001) + fac011*absb(ig,id011)    &
     &              +  fac101*absb(ig,id101) + fac111*absb(ig,id111))
 
          taug(ns04+ig,k) =  tau_major + tau_major1
 
          fracs(ns04+ig,k) = fracrefb(ig,jpl) + fpl                     &
     &                     * (fracrefb(ig,jplp) - fracrefb(ig,jpl))
        enddo
 
!  --- ...  empirical modification to code to improve stratospheric cooling rates
!           for co2. revised to apply weighting for g-point reduction in this band.
 
        taug(ns04+ 8,k) = taug(ns04+ 8,k) * 0.92
        taug(ns04+ 9,k) = taug(ns04+ 9,k) * 0.88
        taug(ns04+10,k) = taug(ns04+10,k) * 1.07
        taug(ns04+11,k) = taug(ns04+11,k) * 1.1
        taug(ns04+12,k) = taug(ns04+12,k) * 0.99
        taug(ns04+13,k) = taug(ns04+13,k) * 0.88
        taug(ns04+14,k) = taug(ns04+14,k) * 0.943
      enddo
 
! ..................................
      end subroutine taugb04
! ----------------------------------
 
! ----------------------------------
      subroutine taugb05
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 5:  700-820 cm-1 (low key - h2o,co2; low minor - o3, ccl4)  !
!                           (high key - o3,co2)                        !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb05
 
!  ---  locals:
      integer :: k, ind0, ind1, inds, indsp, indf, indfp, indm, indmp,  &
     &       id000, id010, id100, id110, id200, id210, jmo3, jmo3p,     &
     &       id001, id011, id101, id111, id201, id211, jpl, jplp,       &
     &       ig, js, js1
 
      real (kind=kind_phys)  :: tauself, taufor, o3m1, o3m2, abso3,     &
     &      speccomb,       specparm,       specmult,       fs,         &
     &      speccomb1,      specparm1,      specmult1,      fs1,        &
     &      speccomb_mo3,   specparm_mo3,   specmult_mo3,   fmo3,       &
     &      speccomb_planck,specparm_planck,specmult_planck,fpl,        &
     &      refrat_planck_a, refrat_planck_b, refrat_m_a,               &
     &      fac000, fac100, fac200, fac010, fac110, fac210,             &
     &      fac001, fac101, fac201, fac011, fac111, fac211,             &
     &      p0, p40, fk00, fk10, fk20, p1, p41, fk01, fk11, fk21
!
!===> ...  begin here
!
!  --- ...  minor gas mapping level :
!     lower - o3, p = 317.34 mbar, t = 240.77 k
!     lower - ccl4
 
!  --- ...  calculate reference ratio to be used in calculation of Planck
!           fraction in lower/upper atmosphere.
 
      refrat_planck_a = chi_mls(1,5)/chi_mls(2,5)      ! P = 473.420 mb
      refrat_planck_b = chi_mls(3,43)/chi_mls(2,43)    ! P = 0.2369  mb
      refrat_m_a = chi_mls(1,7)/chi_mls(2,7)           ! P = 317.348 mb
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        speccomb = colamt(k,1) + rfrate(k,1,1)*colamt(k,2)
        specparm = colamt(k,1) / speccomb
        specmult = 8.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(5) + js
 
        speccomb1 = colamt(k,1) + rfrate(k,1,2)*colamt(k,2)
        specparm1 = colamt(k,1) / speccomb1
        specmult1 = 8.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = (jp(k)*5 + (jt1(k)-1)) * nspa(5) + js1
 
        speccomb_mo3 = colamt(k,1) + refrat_m_a*colamt(k,2)
        specparm_mo3 = colamt(k,1) / speccomb_mo3
        specmult_mo3 = 8.0 * min(specparm_mo3, oneminus)
        jmo3 = 1 + int(specmult_mo3)
        fmo3 = mod(specmult_mo3, f_one)
 
        speccomb_planck = colamt(k,1) + refrat_planck_a*colamt(k,2)
        specparm_planck = colamt(k,1) / speccomb_planck
        specmult_planck = 8.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
 
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
        jplp  = jpl  + 1
        jmo3p = jmo3 + 1
 
        if (specparm < 0.125) then
          p0   = fs - f_one
          p40  = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0 + 2
          id210 = ind0 +11
        elseif (specparm > 0.875) then
          p0   = -fs
          p40  = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0 + 1
          id010 = ind0 +10
          id100 = ind0
          id110 = ind0 + 9
          id200 = ind0 - 1
          id210 = ind0 + 8
        else
          fk00 = f_one - fs
          fk10 = fs
          fk20 = f_zero
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0
          id210 = ind0
        endif
 
        fac000 = fk00 * fac00(k)
        fac100 = fk10 * fac00(k)
        fac200 = fk20 * fac00(k)
        fac010 = fk00 * fac10(k)
        fac110 = fk10 * fac10(k)
        fac210 = fk20 * fac10(k)
 
        if (specparm1 < 0.125) then
          p1   = fs1 - f_one
          p41  = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1 + 2
          id211 = ind1 +11
        elseif (specparm1 > 0.875) then
          p1   = -fs1
          p41  = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1 + 1
          id011 = ind1 +10
          id101 = ind1
          id111 = ind1 + 9
          id201 = ind1 - 1
          id211 = ind1 + 8
        else
          fk01 = f_one - fs1
          fk11 = fs1
          fk21 = f_zero
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1
          id211 = ind1
        endif
 
        fac001 = fk01 * fac01(k)
        fac101 = fk11 * fac01(k)
        fac201 = fk21 * fac01(k)
        fac011 = fk01 * fac11(k)
        fac111 = fk11 * fac11(k)
        fac211 = fk21 * fac11(k)
 
        do ig = 1, ng05
          tauself = selffac(k) * (selfref(ig,inds) + selffrac(k)        &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
          o3m1    = ka_mo3(ig,jmo3,indm) + fmo3                         &
     &            * (ka_mo3(ig,jmo3p,indm) -  ka_mo3(ig,jmo3,indm))
          o3m2    = ka_mo3(ig,jmo3,indmp) + fmo3                        &
     &            * (ka_mo3(ig,jmo3p,indmp) - ka_mo3(ig,jmo3,indmp))
          abso3   = o3m1 + minorfrac(k)*(o3m2 - o3m1)
 
          taug(ns05+ig,k) = speccomb                                    &
     &            * (fac000*absa(ig,id000) + fac010*absa(ig,id010)      &
     &            +  fac100*absa(ig,id100) + fac110*absa(ig,id110)      &
     &            +  fac200*absa(ig,id200) + fac210*absa(ig,id210))     &
     &            +     speccomb1                                       &
     &            * (fac001*absa(ig,id001) + fac011*absa(ig,id011)      &
     &            +  fac101*absa(ig,id101) + fac111*absa(ig,id111)      &
     &            +  fac201*absa(ig,id201) + fac211*absa(ig,id211))     &
     &            + tauself + taufor+abso3*colamt(k,3)+wx(k,1)*ccl4(ig)
 
          fracs(ns05+ig,k) = fracrefa(ig,jpl) + fpl                     &
     &                     * (fracrefa(ig,jplp) - fracrefa(ig,jpl))
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        speccomb = colamt(k,3) + rfrate(k,6,1)*colamt(k,2)
        specparm = colamt(k,3) / speccomb
        specmult = 4.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(5) + js
 
        speccomb1 = colamt(k,3) + rfrate(k,6,2)*colamt(k,2)
        specparm1 = colamt(k,3) / speccomb1
        specmult1 = 4.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(5) + js1
 
        speccomb_planck = colamt(k,3) + refrat_planck_b*colamt(k,2)
        specparm_planck = colamt(k,3) / speccomb_planck
        specmult_planck = 4.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
        jplp= jpl + 1
 
        id000 = ind0
        id010 = ind0 + 5
        id100 = ind0 + 1
        id110 = ind0 + 6
        id001 = ind1
        id011 = ind1 + 5
        id101 = ind1 + 1
        id111 = ind1 + 6
 
        fk00 = f_one - fs
        fk10 = fs
 
        fk01 = f_one - fs1
        fk11 = fs1
 
        fac000 = fk00 * fac00(k)
        fac010 = fk00 * fac10(k)
        fac100 = fk10 * fac00(k)
        fac110 = fk10 * fac10(k)
 
        fac001 = fk01 * fac01(k)
        fac011 = fk01 * fac11(k)
        fac101 = fk11 * fac01(k)
        fac111 = fk11 * fac11(k)
 
        do ig = 1, ng05
          taug(ns05+ig,k) = speccomb                                    &
     &                * (fac000*absb(ig,id000) + fac010*absb(ig,id010)  &
     &                +  fac100*absb(ig,id100) + fac110*absb(ig,id110)) &
     &                +     speccomb1                                   &
     &                * (fac001*absb(ig,id001) + fac011*absb(ig,id011)  &
     &                +  fac101*absb(ig,id101) + fac111*absb(ig,id111)) &
     &                + wx(k,1) * ccl4(ig)
 
          fracs(ns05+ig,k) = fracrefb(ig,jpl) + fpl                     &
     &                     * (fracrefb(ig,jplp) - fracrefb(ig,jpl))
        enddo
      enddo
 
! ..................................
      end subroutine taugb05
! ----------------------------------
 
! ----------------------------------
      subroutine taugb06
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 6:  820-980 cm-1 (low key - h2o; low minor - co2)           !
!                           (high key - none; high minor - cfc11, cfc12)
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb06
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &       indm, indmp, ig
 
      real (kind=kind_phys) :: ratco2, adjfac, adjcolco2, tauself,      &
     &      taufor, absco2, temp
!
!===> ...  begin here
!
!  --- ...  minor gas mapping level:
!     lower - co2, p = 706.2720 mb, t = 294.2 k
!     upper - cfc11, cfc12
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(6) + 1
        ind1 = ( jp(k)   *5 + (jt1(k)-1)) * nspa(6) + 1
 
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
        ind0p = ind0 + 1
        ind1p = ind1 + 1
 
!  --- ...  in atmospheres where the amount of co2 is too great to be considered
!           a minor species, adjust the column amount of co2 by an empirical factor
!           to obtain the proper contribution.
 
        temp   = coldry(k) * chi_mls(2,jp(k)+1)
        ratco2 = colamt(k,2) / temp
        if (ratco2 > 3.0) then
          adjfac = 2.0 + (ratco2-2.0)**0.77
          adjcolco2 = adjfac * temp
        else
          adjcolco2 = colamt(k,2)
        endif
 
        do ig = 1, ng06
          tauself = selffac(k) * (selfref(ig,inds) + selffrac(k)        &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
          absco2  = ka_mco2(ig,indm) + minorfrac(k)                     &
     &            * (ka_mco2(ig,indmp) - ka_mco2(ig,indm))
 
          taug(ns06+ig,k) = colamt(k,1)                                 &
     &            * (fac00(k)*absa(ig,ind0) + fac10(k)*absa(ig,ind0p)   &
     &            +  fac01(k)*absa(ig,ind1) + fac11(k)*absa(ig,ind1p))  &
     &            +  tauself + taufor + adjcolco2*absco2                &
     &            +  wx(k,2)*cfc11adj(ig) + wx(k,3)*cfc12(ig)
 
          fracs(ns06+ig,k) = fracrefa(ig)
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
!           nothing important goes on above laytrop in this band.
 
      do k = laytrop+1, nlay
        do ig = 1, ng06
          taug(ns06+ig,k) = wx(k,2)*cfc11adj(ig) + wx(k,3)*cfc12(ig)
 
          fracs(ns06+ig,k) = fracrefa(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb06
! ----------------------------------
 
! ----------------------------------
      subroutine taugb07
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 7:  980-1080 cm-1 (low key - h2o,o3; low minor - co2)       !
!                            (high key - o3; high minor - co2)         !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb07
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &       id000, id010, id100, id110, id200, id210, indm, indmp,     &
     &       id001, id011, id101, id111, id201, id211, jmco2, jmco2p,   &
     &       jpl, jplp, ig, js, js1
 
      real (kind=kind_phys) :: tauself, taufor, co2m1, co2m2, absco2,   &
     &      speccomb,       specparm,       specmult,       fs,         &
     &      speccomb1,      specparm1,      specmult1,      fs1,        &
     &      speccomb_mco2,  specparm_mco2,  specmult_mco2,  fmco2,      &
     &      speccomb_planck,specparm_planck,specmult_planck,fpl,        &
     &      refrat_planck_a, refrat_m_a, ratco2, adjfac, adjcolco2,     &
     &      fac000, fac100, fac200, fac010, fac110, fac210,             &
     &      fac001, fac101, fac201, fac011, fac111, fac211,             &
     &      p0, p40, fk00, fk10, fk20, p1, p41, fk01, fk11, fk21, temp
!
!===> ...  begin here
!
!  --- ...  minor gas mapping level :
!     lower - co2, p = 706.2620 mbar, t= 278.94 k
!     upper - co2, p = 12.9350 mbar, t = 234.01 k
 
!  --- ...  calculate reference ratio to be used in calculation of Planck
!           fraction in lower atmosphere.
 
      refrat_planck_a = chi_mls(1,3)/chi_mls(3,3)     ! P = 706.2620 mb
      refrat_m_a = chi_mls(1,3)/chi_mls(3,3)          ! P = 706.2720 mb
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        speccomb = colamt(k,1) + rfrate(k,2,1)*colamt(k,3)
        specparm = colamt(k,1) / speccomb
        specmult = 8.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(7) + js
 
        speccomb1 = colamt(k,1) + rfrate(k,2,2)*colamt(k,3)
        specparm1 = colamt(k,1) / speccomb1
        specmult1 = 8.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = (jp(k)*5 + (jt1(k)-1)) * nspa(7) + js1
 
        speccomb_mco2 = colamt(k,1) + refrat_m_a*colamt(k,3)
        specparm_mco2 = colamt(k,1) / speccomb_mco2
        specmult_mco2 = 8.0 * min(specparm_mco2, oneminus)
        jmco2 = 1 + int(specmult_mco2)
        fmco2 = mod(specmult_mco2, f_one)
 
        speccomb_planck = colamt(k,1) + refrat_planck_a*colamt(k,3)
        specparm_planck = colamt(k,1) / speccomb_planck
        specmult_planck = 8.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
 
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
        jplp  = jpl  + 1
        jmco2p= jmco2+ 1
        ind0p = ind0 + 1
        ind1p = ind1 + 1
 
!  --- ...  in atmospheres where the amount of CO2 is too great to be considered
!           a minor species, adjust the column amount of CO2 by an empirical factor
!           to obtain the proper contribution.
 
        temp   = coldry(k) * chi_mls(2,jp(k)+1)
        ratco2 = colamt(k,2) / temp
        if (ratco2 > 3.0) then
          adjfac = 3.0 + (ratco2-3.0)**0.79
          adjcolco2 = adjfac * temp
        else
          adjcolco2 = colamt(k,2)
        endif
 
        if (specparm < 0.125) then
          p0 = fs - f_one
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0 + 2
          id210 = ind0 +11
        elseif (specparm > 0.875) then
          p0 = -fs
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0 + 1
          id010 = ind0 +10
          id100 = ind0
          id110 = ind0 + 9
          id200 = ind0 - 1
          id210 = ind0 + 8
        else
          fk00 = f_one - fs
          fk10 = fs
          fk20 = f_zero
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0
          id210 = ind0
        endif
 
        fac000 = fk00 * fac00(k)
        fac100 = fk10 * fac00(k)
        fac200 = fk20 * fac00(k)
        fac010 = fk00 * fac10(k)
        fac110 = fk10 * fac10(k)
        fac210 = fk20 * fac10(k)
 
        if (specparm1 < 0.125) then
          p1 = fs1 - f_one
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1 + 2
          id211 = ind1 +11
        elseif (specparm1 > 0.875) then
          p1 = -fs1
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1 + 1
          id011 = ind1 +10
          id101 = ind1
          id111 = ind1 + 9
          id201 = ind1 - 1
          id211 = ind1 + 8
        else
          fk01 = f_one - fs1
          fk11 = fs1
          fk21 = f_zero
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1
          id211 = ind1
        endif
 
        fac001 = fk01 * fac01(k)
        fac101 = fk11 * fac01(k)
        fac201 = fk21 * fac01(k)
        fac011 = fk01 * fac11(k)
        fac111 = fk11 * fac11(k)
        fac211 = fk21 * fac11(k)
 
        do ig = 1, ng07
          tauself = selffac(k)* (selfref(ig,inds) + selffrac(k)         &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
          co2m1   = ka_mco2(ig,jmco2,indm) + fmco2                      &
     &            * (ka_mco2(ig,jmco2p,indm) - ka_mco2(ig,jmco2,indm))
          co2m2   = ka_mco2(ig,jmco2,indmp) + fmco2                     &
     &            * (ka_mco2(ig,jmco2p,indmp) - ka_mco2(ig,jmco2,indmp))
          absco2  = co2m1 + minorfrac(k) * (co2m2 - co2m1)
 
          taug(ns07+ig,k) = speccomb                                    &
     &                * (fac000*absa(ig,id000) + fac010*absa(ig,id010)  &
     &                +  fac100*absa(ig,id100) + fac110*absa(ig,id110)  &
     &                +  fac200*absa(ig,id200) + fac210*absa(ig,id210)) &
     &                +     speccomb1                                   &
     &                * (fac001*absa(ig,id001) + fac011*absa(ig,id011)  &
     &                +  fac101*absa(ig,id101) + fac111*absa(ig,id111)  &
     &                +  fac201*absa(ig,id201) + fac211*absa(ig,id211)) &
     &                + tauself + taufor + adjcolco2*absco2
 
          fracs(ns07+ig,k) = fracrefa(ig,jpl) + fpl                     &
     &                     * (fracrefa(ig,jplp) - fracrefa(ig,jpl))
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
!  --- ...  in atmospheres where the amount of co2 is too great to be considered
!           a minor species, adjust the column amount of co2 by an empirical factor
!           to obtain the proper contribution.
 
      do k = laytrop+1, nlay
        temp   = coldry(k) * chi_mls(2,jp(k)+1)
        ratco2 = colamt(k,2) / temp
        if (ratco2 > 3.0) then
          adjfac = 2.0 + (ratco2-2.0)**0.79
          adjcolco2 = adjfac * temp
        else
          adjcolco2 = colamt(k,2)
        endif
 
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(7) + 1
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(7) + 1
 
        indm = indminor(k)
        indmp = indm + 1
        ind0p = ind0 + 1
        ind1p = ind1 + 1
 
        do ig = 1, ng07
          absco2 = kb_mco2(ig,indm) + minorfrac(k)                      &
     &           * (kb_mco2(ig,indmp) - kb_mco2(ig,indm))
 
          taug(ns07+ig,k) = colamt(k,3)                                 &
     &            * (fac00(k)*absb(ig,ind0) + fac10(k)*absb(ig,ind0p)   &
     &            +  fac01(k)*absb(ig,ind1) + fac11(k)*absb(ig,ind1p))  &
     &            + adjcolco2 * absco2
 
          fracs(ns07+ig,k) = fracrefb(ig)
        enddo
 
!  --- ...  empirical modification to code to improve stratospheric cooling rates
!           for o3.  revised to apply weighting for g-point reduction in this band.
 
        taug(ns07+ 6,k) = taug(ns07+ 6,k) * 0.92
        taug(ns07+ 7,k) = taug(ns07+ 7,k) * 0.88
        taug(ns07+ 8,k) = taug(ns07+ 8,k) * 1.07
        taug(ns07+ 9,k) = taug(ns07+ 9,k) * 1.1
        taug(ns07+10,k) = taug(ns07+10,k) * 0.99
        taug(ns07+11,k) = taug(ns07+11,k) * 0.855
      enddo
 
! ..................................
      end subroutine taugb07
! ----------------------------------
 
! ----------------------------------
      subroutine taugb08
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 8:  1080-1180 cm-1 (low key - h2o; low minor - co2,o3,n2o)  !
!                             (high key - o3; high minor - co2, n2o)   !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb08
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &       indm, indmp, ig
 
      real (kind=kind_phys) :: tauself, taufor, absco2, abso3, absn2o,  &
     &      ratco2, adjfac, adjcolco2, temp
!
!===> ...  begin here
!
!  --- ...  minor gas mapping level:
!     lower - co2, p = 1053.63 mb, t = 294.2 k
!     lower - o3,  p = 317.348 mb, t = 240.77 k
!     lower - n2o, p = 706.2720 mb, t= 278.94 k
!     lower - cfc12,cfc11
!     upper - co2, p = 35.1632 mb, t = 223.28 k
!     upper - n2o, p = 8.716e-2 mb, t = 226.03 k
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(8) + 1
        ind1 = ( jp(k)   *5 + (jt1(k)-1)) * nspa(8) + 1
 
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
 
!  --- ...  in atmospheres where the amount of co2 is too great to be considered
!           a minor species, adjust the column amount of co2 by an empirical factor
!           to obtain the proper contribution.
 
        temp   = coldry(k) * chi_mls(2,jp(k)+1)
        ratco2 = colamt(k,2) / temp
        if (ratco2 > 3.0) then
          adjfac = 2.0 + (ratco2-2.0)**0.65
          adjcolco2 = adjfac * temp
        else
          adjcolco2 = colamt(k,2)
        endif
 
        do ig = 1, ng08
          tauself = selffac(k) * (selfref(ig,inds) + selffrac(k)        &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
          absco2  = (ka_mco2(ig,indm) + minorfrac(k)                    &
     &            * (ka_mco2(ig,indmp) - ka_mco2(ig,indm)))
          abso3   = (ka_mo3(ig,indm) + minorfrac(k)                     &
     &            * (ka_mo3(ig,indmp) - ka_mo3(ig,indm)))
          absn2o  = (ka_mn2o(ig,indm) + minorfrac(k)                    &
     &            * (ka_mn2o(ig,indmp) - ka_mn2o(ig,indm)))
 
          taug(ns08+ig,k) = colamt(k,1)                                 &
     &            * (fac00(k)*absa(ig,ind0) + fac10(k)*absa(ig,ind0p)   &
     &            +  fac01(k)*absa(ig,ind1) + fac11(k)*absa(ig,ind1p))  &
     &            + tauself+taufor + adjcolco2*absco2                   &
     &            + colamt(k,3)*abso3 + colamt(k,4)*absn2o              &
     &            + wx(k,3)*cfc12(ig) + wx(k,4)*cfc22adj(ig)
 
          fracs(ns08+ig,k) = fracrefa(ig)
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(8) + 1
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(8) + 1
 
        indm = indminor(k)
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indmp = indm + 1
 
!  --- ...  in atmospheres where the amount of co2 is too great to be considered
!           a minor species, adjust the column amount of co2 by an empirical factor
!           to obtain the proper contribution.
 
        temp   = coldry(k) * chi_mls(2,jp(k)+1)
        ratco2 = colamt(k,2) / temp
        if (ratco2 > 3.0) then
          adjfac = 2.0 + (ratco2-2.0)**0.65
          adjcolco2 = adjfac * temp
        else
          adjcolco2 = colamt(k,2)
        endif
 
        do ig = 1, ng08
          absco2 = (kb_mco2(ig,indm) + minorfrac(k)                     &
     &           * (kb_mco2(ig,indmp) - kb_mco2(ig,indm)))
          absn2o = (kb_mn2o(ig,indm) + minorfrac(k)                     &
     &           * (kb_mn2o(ig,indmp) - kb_mn2o(ig,indm)))
 
          taug(ns08+ig,k) = colamt(k,3)                                 &
     &           * (fac00(k)*absb(ig,ind0) + fac10(k)*absb(ig,ind0p)    &
     &           +  fac01(k)*absb(ig,ind1) + fac11(k)*absb(ig,ind1p))   &
     &           + adjcolco2*absco2 + colamt(k,4)*absn2o                &
     &           + wx(k,3)*cfc12(ig) + wx(k,4)*cfc22adj(ig)
 
          fracs(ns08+ig,k) = fracrefb(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb08
! ----------------------------------
 
! ----------------------------------
      subroutine taugb09
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 9:  1180-1390 cm-1 (low key - h2o,ch4; low minor - n2o)     !
!                             (high key - ch4; high minor - n2o)       !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb09
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &       id000, id010, id100, id110, id200, id210, indm, indmp,     &
     &       id001, id011, id101, id111, id201, id211, jmn2o, jmn2op,   &
     &       jpl, jplp, ig, js, js1
 
      real (kind=kind_phys) :: tauself, taufor, n2om1, n2om2, absn2o,   &
     &       speccomb,       specparm,       specmult,       fs,        &
     &       speccomb1,      specparm1,      specmult1,      fs1,       &
     &       speccomb_mn2o,  specparm_mn2o,  specmult_mn2o,  fmn2o,     &
     &       speccomb_planck,specparm_planck,specmult_planck,fpl,       &
     &       refrat_planck_a, refrat_m_a, ratn2o, adjfac, adjcoln2o,    &
     &       fac000, fac100, fac200, fac010, fac110, fac210,            &
     &       fac001, fac101, fac201, fac011, fac111, fac211,            &
     &       p0, p40, fk00, fk10, fk20, p1, p41, fk01, fk11, fk21, temp
!
!===> ...  begin here
!
!  --- ...  minor gas mapping level :
!     lower - n2o, p = 706.272 mbar, t = 278.94 k
!     upper - n2o, p = 95.58 mbar, t = 215.7 k
 
!  --- ...  calculate reference ratio to be used in calculation of Planck
!           fraction in lower/upper atmosphere.
 
      refrat_planck_a = chi_mls(1,9)/chi_mls(6,9)       ! P = 212 mb
      refrat_m_a = chi_mls(1,3)/chi_mls(6,3)            ! P = 706.272 mb
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        speccomb = colamt(k,1) + rfrate(k,4,1)*colamt(k,5)
        specparm = colamt(k,1) / speccomb
        specmult = 8.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(9) + js
 
        speccomb1 = colamt(k,1) + rfrate(k,4,2)*colamt(k,5)
        specparm1 = colamt(k,1) / speccomb1
        specmult1 = 8.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = (jp(k)*5 + (jt1(k)-1)) * nspa(9) + js1
 
        speccomb_mn2o = colamt(k,1) + refrat_m_a*colamt(k,5)
        specparm_mn2o = colamt(k,1) / speccomb_mn2o
        specmult_mn2o = 8.0 * min(specparm_mn2o, oneminus)
        jmn2o = 1 + int(specmult_mn2o)
        fmn2o = mod(specmult_mn2o, f_one)
 
        speccomb_planck = colamt(k,1) + refrat_planck_a*colamt(k,5)
        specparm_planck = colamt(k,1) / speccomb_planck
        specmult_planck = 8.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
 
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
        jplp  = jpl  + 1
        jmn2op= jmn2o+ 1
 
!  --- ...  in atmospheres where the amount of n2o is too great to be considered
!           a minor species, adjust the column amount of n2o by an empirical factor
!           to obtain the proper contribution.
 
        temp   = coldry(k) * chi_mls(4,jp(k)+1)
        ratn2o = colamt(k,4) / temp
        if (ratn2o > 1.5) then
          adjfac = 0.5 + (ratn2o-0.5)**0.65
          adjcoln2o = adjfac * temp
        else
          adjcoln2o = colamt(k,4)
        endif
 
        if (specparm < 0.125) then
          p0 = fs - f_one
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0 + 2
          id210 = ind0 +11
        elseif (specparm > 0.875) then
          p0 = -fs
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0 + 1
          id010 = ind0 +10
          id100 = ind0
          id110 = ind0 + 9
          id200 = ind0 - 1
          id210 = ind0 + 8
        else
          fk00 = f_one - fs
          fk10 = fs
          fk20 = f_zero
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0
          id210 = ind0
        endif
 
        fac000 = fk00 * fac00(k)
        fac100 = fk10 * fac00(k)
        fac200 = fk20 * fac00(k)
        fac010 = fk00 * fac10(k)
        fac110 = fk10 * fac10(k)
        fac210 = fk20 * fac10(k)
 
        if (specparm1 < 0.125) then
          p1 = fs1 - f_one
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1 + 2
          id211 = ind1 +11
        elseif (specparm1 > 0.875) then
          p1 = -fs1
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1 + 1
          id011 = ind1 +10
          id101 = ind1
          id111 = ind1 + 9
          id201 = ind1 - 1
          id211 = ind1 + 8
        else
          fk01 = f_one - fs1
          fk11 = fs1
          fk21 = f_zero
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1
          id211 = ind1
        endif
 
        fac001 = fk01 * fac01(k)
        fac101 = fk11 * fac01(k)
        fac201 = fk21 * fac01(k)
        fac011 = fk01 * fac11(k)
        fac111 = fk11 * fac11(k)
        fac211 = fk21 * fac11(k)
 
        do ig = 1, ng09
          tauself = selffac(k)* (selfref(ig,inds) + selffrac(k)         &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
          n2om1   = ka_mn2o(ig,jmn2o,indm) + fmn2o                      &
     &            * (ka_mn2o(ig,jmn2op,indm) - ka_mn2o(ig,jmn2o,indm))
          n2om2   = ka_mn2o(ig,jmn2o,indmp) + fmn2o                     &
     &            * (ka_mn2o(ig,jmn2op,indmp) - ka_mn2o(ig,jmn2o,indmp))
          absn2o  = n2om1 + minorfrac(k) * (n2om2 - n2om1)
 
          taug(ns09+ig,k) = speccomb                                    &
     &                * (fac000*absa(ig,id000) + fac010*absa(ig,id010)  &
     &                +  fac100*absa(ig,id100) + fac110*absa(ig,id110)  &
     &                +  fac200*absa(ig,id200) + fac210*absa(ig,id210)) &
     &                +     speccomb1                                   &
     &                * (fac001*absa(ig,id001) + fac011*absa(ig,id011)  &
     &                +  fac101*absa(ig,id101) + fac111*absa(ig,id111)  &
     &                +  fac201*absa(ig,id201) + fac211*absa(ig,id211)) &
     &                + tauself + taufor + adjcoln2o*absn2o
 
          fracs(ns09+ig,k) = fracrefa(ig,jpl) + fpl                     &
     &                     * (fracrefa(ig,jplp) - fracrefa(ig,jpl))
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(9) + 1
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(9) + 1
 
        indm = indminor(k)
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indmp = indm + 1
 
!  --- ...  in atmospheres where the amount of n2o is too great to be considered
!           a minor species, adjust the column amount of n2o by an empirical factor
!           to obtain the proper contribution.
 
        temp   = coldry(k) * chi_mls(4,jp(k)+1)
        ratn2o = colamt(k,4) / temp
        if (ratn2o > 1.5) then
          adjfac = 0.5 + (ratn2o - 0.5)**0.65
          adjcoln2o = adjfac * temp
        else
          adjcoln2o = colamt(k,4)
        endif
 
        do ig = 1, ng09
          absn2o = kb_mn2o(ig,indm) + minorfrac(k)                      &
     &           * (kb_mn2o(ig,indmp) - kb_mn2o(ig,indm))
 
          taug(ns09+ig,k) = colamt(k,5)                                 &
     &           * (fac00(k)*absb(ig,ind0) + fac10(k)*absb(ig,ind0p)    &
     &           +  fac01(k)*absb(ig,ind1) + fac11(k)*absb(ig,ind1p))   &
     &           + adjcoln2o*absn2o
 
          fracs(ns09+ig,k) = fracrefb(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb09
! ----------------------------------
 
! ----------------------------------
      subroutine taugb10
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 10:  1390-1480 cm-1 (low key - h2o; high key - h2o)         !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb10
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &       ig
 
      real (kind=kind_phys) :: tauself, taufor
!
!===> ...  begin here
!
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(10) + 1
        ind1 = ( jp(k)   *5 + (jt1(k)-1)) * nspa(10) + 1
 
        inds = indself(k)
        indf = indfor(k)
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indsp = inds + 1
        indfp = indf + 1
 
        do ig = 1, ng10
          tauself = selffac(k) * (selfref(ig,inds) + selffrac(k)        &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
 
          taug(ns10+ig,k) = colamt(k,1)                                 &
     &            * (fac00(k)*absa(ig,ind0) + fac10(k)*absa(ig,ind0p)   &
     &            +  fac01(k)*absa(ig,ind1) + fac11(k)*absa(ig,ind1p))  &
     &            + tauself + taufor
 
          fracs(ns10+ig,k) = fracrefa(ig)
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(10) + 1
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(10) + 1
 
        indf = indfor(k)
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indfp = indf + 1
 
        do ig = 1, ng10
          taufor = forfac(k) * (forref(ig,indf) + forfrac(k)            &
     &           * (forref(ig,indfp) - forref(ig,indf)))
 
          taug(ns10+ig,k) = colamt(k,1)                                 &
     &            * (fac00(k)*absb(ig,ind0) + fac10(k)*absb(ig,ind0p)   &
     &            +  fac01(k)*absb(ig,ind1) + fac11(k)*absb(ig,ind1p))  &
     &            + taufor
 
          fracs(ns10+ig,k) = fracrefb(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb10
! ----------------------------------
 
! ----------------------------------
      subroutine taugb11
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 11:  1480-1800 cm-1 (low - h2o; low minor - o2)             !
!                              (high key - h2o; high minor - o2)       !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb11
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &       indm, indmp, ig
 
      real (kind=kind_phys) :: scaleo2, tauself, taufor, tauo2
!
!===> ...  begin here
!
!  --- ...  minor gas mapping level :
!     lower - o2, p = 706.2720 mbar, t = 278.94 k
!     upper - o2, p = 4.758820 mbarm t = 250.85 k
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(11) + 1
        ind1 = ( jp(k)   *5 + (jt1(k)-1)) * nspa(11) + 1
 
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
 
        scaleo2 = colamt(k,6) * scaleminor(k)
 
        do ig = 1, ng11
          tauself = selffac(k) * (selfref(ig,inds) + selffrac(k)        &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
          tauo2   = scaleo2 * (ka_mo2(ig,indm) + minorfrac(k)           &
     &            * (ka_mo2(ig,indmp) - ka_mo2(ig,indm)))
 
          taug(ns11+ig,k) = colamt(k,1)                                 &
     &            * (fac00(k)*absa(ig,ind0) + fac10(k)*absa(ig,ind0p)   &
     &            +  fac01(k)*absa(ig,ind1) + fac11(k)*absa(ig,ind1p))  &
     &            + tauself + taufor + tauo2
 
          fracs(ns11+ig,k) = fracrefa(ig)
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(11) + 1
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(11) + 1
 
        indf = indfor(k)
        indm = indminor(k)
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indfp = indf + 1
        indmp = indm + 1
 
        scaleo2 = colamt(k,6) * scaleminor(k)
 
        do ig = 1, ng11
          taufor = forfac(k) * (forref(ig,indf) + forfrac(k)            &
     &           * (forref(ig,indfp) - forref(ig,indf)))
          tauo2  = scaleo2 * (kb_mo2(ig,indm) + minorfrac(k)            &
     &           * (kb_mo2(ig,indmp) - kb_mo2(ig,indm)))
 
          taug(ns11+ig,k) = colamt(k,1)                                 &
     &            * (fac00(k)*absb(ig,ind0) + fac10(k)*absb(ig,ind0p)   &
     &            +  fac01(k)*absb(ig,ind1) + fac11(k)*absb(ig,ind1p))  &
     &            + taufor + tauo2
 
          fracs(ns11+ig,k) = fracrefb(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb11
! ----------------------------------
 
! ----------------------------------
      subroutine taugb12
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 12:  1800-2080 cm-1 (low - h2o,co2; high - nothing)         !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb12
 
!  ---  locals:
      integer :: k, ind0, ind1, inds, indsp, indf, indfp, jpl, jplp,    &
     &       id000, id010, id100, id110, id200, id210, ig, js, js1,     &
     &       id001, id011, id101, id111, id201, id211
 
      real (kind=kind_phys) :: tauself, taufor, refrat_planck_a,        &
     &       speccomb,       specparm,       specmult,       fs,        &
     &       speccomb1,      specparm1,      specmult1,      fs1,       &
     &       speccomb_planck,specparm_planck,specmult_planck,fpl,       &
     &       fac000, fac100, fac200, fac010, fac110, fac210,            &
     &       fac001, fac101, fac201, fac011, fac111, fac211,            &
     &       p0, p40, fk00, fk10, fk20, p1, p41, fk01, fk11, fk21
!
!===> ...  begin here
!
!  --- ...  calculate reference ratio to be used in calculation of Planck
!           fraction in lower/upper atmosphere.
 
      refrat_planck_a = chi_mls(1,10)/chi_mls(2,10)      ! P =   174.164 mb
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        speccomb = colamt(k,1) + rfrate(k,1,1)*colamt(k,2)
        specparm = colamt(k,1) / speccomb
        specmult = 8.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(12) + js
 
        speccomb1 = colamt(k,1) + rfrate(k,1,2)*colamt(k,2)
        specparm1 = colamt(k,1) / speccomb1
        specmult1 = 8.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = (jp(k)*5 + (jt1(k)-1)) * nspa(12) + js1
 
        speccomb_planck = colamt(k,1) + refrat_planck_a*colamt(k,2)
        specparm_planck = colamt(k,1) / speccomb_planck
        if (specparm_planck >= oneminus) specparm_planck=oneminus
        specmult_planck = 8.0 * specparm_planck
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
 
        inds = indself(k)
        indf = indfor(k)
        indsp = inds + 1
        indfp = indf + 1
        jplp  = jpl  + 1
 
        if (specparm < 0.125) then
          p0 = fs - f_one
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0 + 2
          id210 = ind0 +11
        elseif (specparm > 0.875) then
          p0 = -fs
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0 + 1
          id010 = ind0 +10
          id100 = ind0
          id110 = ind0 + 9
          id200 = ind0 - 1
          id210 = ind0 + 8
        else
          fk00 = f_one - fs
          fk10 = fs
          fk20 = f_zero
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0
          id210 = ind0
        endif
 
        fac000 = fk00 * fac00(k)
        fac100 = fk10 * fac00(k)
        fac200 = fk20 * fac00(k)
        fac010 = fk00 * fac10(k)
        fac110 = fk10 * fac10(k)
        fac210 = fk20 * fac10(k)
 
        if (specparm1 < 0.125) then
          p1 = fs1 - f_one
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1 + 2
          id211 = ind1 +11
        elseif (specparm1 > 0.875) then
          p1 = -fs1
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1 + 1
          id011 = ind1 +10
          id101 = ind1
          id111 = ind1 + 9
          id201 = ind1 - 1
          id211 = ind1 + 8
        else
          fk01 = f_one - fs1
          fk11 = fs1
          fk21 = f_zero
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1
          id211 = ind1
        endif
 
        fac001 = fk01 * fac01(k)
        fac101 = fk11 * fac01(k)
        fac201 = fk21 * fac01(k)
        fac011 = fk01 * fac11(k)
        fac111 = fk11 * fac11(k)
        fac211 = fk21 * fac11(k)
 
        do ig = 1, ng12
          tauself = selffac(k)* (selfref(ig,inds) + selffrac(k)         &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
 
          taug(ns12+ig,k) = speccomb                                    &
     &                * (fac000*absa(ig,id000) + fac010*absa(ig,id010)  &
     &                +  fac100*absa(ig,id100) + fac110*absa(ig,id110)  &
     &                +  fac200*absa(ig,id200) + fac210*absa(ig,id210)) &
     &                +     speccomb1                                   &
     &                * (fac001*absa(ig,id001) + fac011*absa(ig,id011)  &
     &                +  fac101*absa(ig,id101) + fac111*absa(ig,id111)  &
     &                +  fac201*absa(ig,id201) + fac211*absa(ig,id211)) &
     &                + tauself + taufor
 
          fracs(ns12+ig,k) = fracrefa(ig,jpl) + fpl                     &
     &                     *(fracrefa(ig,jplp) - fracrefa(ig,jpl))
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        do ig = 1, ng12
          taug(ns12+ig,k) = f_zero
          fracs(ns12+ig,k) = f_zero
        enddo
      enddo
 
! ..................................
      end subroutine taugb12
! ----------------------------------
 
! ----------------------------------
      subroutine taugb13
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 13:  2080-2250 cm-1 (low key-h2o,n2o; high minor-o3 minor)  !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb13
 
!  ---  locals:
      integer :: k, ind0, ind1, inds, indsp, indf, indfp, indm, indmp,  &
     &       id000, id010, id100, id110, id200, id210, jmco2, jpl,      &
     &       id001, id011, id101, id111, id201, id211, jmco2p, jplp,    &
     &       jmco, jmcop, ig, js, js1
 
      real (kind=kind_phys) :: tauself, taufor, co2m1, co2m2, absco2,   &
     &       speccomb,       specparm,       specmult,       fs,        &
     &       speccomb1,      specparm1,      specmult1,      fs1,       &
     &       speccomb_mco2,  specparm_mco2,  specmult_mco2,  fmco2,     &
     &       speccomb_mco,   specparm_mco,   specmult_mco,   fmco,      &
     &       speccomb_planck,specparm_planck,specmult_planck,fpl,       &
     &       refrat_planck_a, refrat_m_a, refrat_m_a3, ratco2,          &
     &       adjfac, adjcolco2, com1, com2, absco, abso3,               &
     &       fac000, fac100, fac200, fac010, fac110, fac210,            &
     &       fac001, fac101, fac201, fac011, fac111, fac211,            &
     &       p0, p40, fk00, fk10, fk20, p1, p41, fk01, fk11, fk21, temp
!
!===> ...  begin here
!
!  --- ...  minor gas mapping levels :
!     lower - co2, p = 1053.63 mb, t = 294.2 k
!     lower - co, p = 706 mb, t = 278.94 k
!     upper - o3, p = 95.5835 mb, t = 215.7 k
 
!  --- ...  calculate reference ratio to be used in calculation of Planck
!           fraction in lower/upper atmosphere.
 
      refrat_planck_a = chi_mls(1,5)/chi_mls(4,5)        ! P = 473.420 mb (Level 5)
      refrat_m_a = chi_mls(1,1)/chi_mls(4,1)             ! P = 1053. (Level 1)
      refrat_m_a3 = chi_mls(1,3)/chi_mls(4,3)            ! P = 706. (Level 3)
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        speccomb = colamt(k,1) + rfrate(k,3,1)*colamt(k,4)
        specparm = colamt(k,1) / speccomb
        specmult = 8.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(13) + js
 
        speccomb1 = colamt(k,1) + rfrate(k,3,2)*colamt(k,4)
        specparm1 = colamt(k,1) / speccomb1
        specmult1 = 8.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = (jp(k)*5 + (jt1(k)-1)) * nspa(13) + js1
 
        speccomb_mco2 = colamt(k,1) + refrat_m_a*colamt(k,4)
        specparm_mco2 = colamt(k,1) / speccomb_mco2
        specmult_mco2 = 8.0 * min(specparm_mco2, oneminus)
        jmco2 = 1 + int(specmult_mco2)
        fmco2 = mod(specmult_mco2, f_one)
 
!  --- ...  in atmospheres where the amount of co2 is too great to be considered
!           a minor species, adjust the column amount of co2 by an empirical factor
!           to obtain the proper contribution.
 
        speccomb_mco = colamt(k,1) + refrat_m_a3*colamt(k,4)
        specparm_mco = colamt(k,1) / speccomb_mco
        specmult_mco = 8.0 * min(specparm_mco, oneminus)
        jmco = 1 + int(specmult_mco)
        fmco = mod(specmult_mco, f_one)
 
        speccomb_planck = colamt(k,1) + refrat_planck_a*colamt(k,4)
        specparm_planck = colamt(k,1) / speccomb_planck
        specmult_planck = 8.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
 
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
        jplp  = jpl  + 1
        jmco2p= jmco2+ 1
        jmcop = jmco + 1
 
!  --- ...  in atmospheres where the amount of co2 is too great to be considered
!           a minor species, adjust the column amount of co2 by an empirical factor
!           to obtain the proper contribution.
 
        temp   = coldry(k) * 3.55e-4
        ratco2 = colamt(k,2) / temp
        if (ratco2 > 3.0) then
          adjfac = 2.0 + (ratco2-2.0)**0.68
          adjcolco2 = adjfac * temp
        else
          adjcolco2 = colamt(k,2)
        endif
 
        if (specparm < 0.125) then
          p0 = fs - f_one
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0 + 2
          id210 = ind0 +11
        elseif (specparm > 0.875) then
          p0 = -fs
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0 + 1
          id010 = ind0 +10
          id100 = ind0
          id110 = ind0 + 9
          id200 = ind0 - 1
          id210 = ind0 + 8
        else
          fk00 = f_one - fs
          fk10 = fs
          fk20 = f_zero
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0
          id210 = ind0
        endif
 
        fac000 = fk00 * fac00(k)
        fac100 = fk10 * fac00(k)
        fac200 = fk20 * fac00(k)
        fac010 = fk00 * fac10(k)
        fac110 = fk10 * fac10(k)
        fac210 = fk20 * fac10(k)
 
        if (specparm1 < 0.125) then
          p1 = fs1 - f_one
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1 + 2
          id211 = ind1 +11
        elseif (specparm1 > 0.875) then
          p1 = -fs1
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1 + 1
          id011 = ind1 +10
          id101 = ind1
          id111 = ind1 + 9
          id201 = ind1 - 1
          id211 = ind1 + 8
        else
          fk01 = f_one - fs1
          fk11 = fs1
          fk21 = f_zero
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1
          id211 = ind1
        endif
 
        fac001 = fk01 * fac01(k)
        fac101 = fk11 * fac01(k)
        fac201 = fk21 * fac01(k)
        fac011 = fk01 * fac11(k)
        fac111 = fk11 * fac11(k)
        fac211 = fk21 * fac11(k)
 
        do ig = 1, ng13
          tauself = selffac(k)* (selfref(ig,inds) + selffrac(k)         &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
          co2m1   = ka_mco2(ig,jmco2,indm) + fmco2                      &
     &            * (ka_mco2(ig,jmco2p,indm) - ka_mco2(ig,jmco2,indm))
          co2m2   = ka_mco2(ig,jmco2,indmp) + fmco2                     &
     &            * (ka_mco2(ig,jmco2p,indmp) - ka_mco2(ig,jmco2,indmp))
          absco2  = co2m1 + minorfrac(k) * (co2m2 - co2m1)
          com1    = ka_mco(ig,jmco,indm) + fmco                         &
     &            * (ka_mco(ig,jmcop,indm) - ka_mco(ig,jmco,indm))
          com2    = ka_mco(ig,jmco,indmp) + fmco                        &
     &            * (ka_mco(ig,jmcop,indmp) - ka_mco(ig,jmco,indmp))
          absco   = com1 + minorfrac(k) * (com2 - com1)
 
          taug(ns13+ig,k) = speccomb                                    &
     &                * (fac000*absa(ig,id000) + fac010*absa(ig,id010)  &
     &                +  fac100*absa(ig,id100) + fac110*absa(ig,id110)  &
     &                +  fac200*absa(ig,id200) + fac210*absa(ig,id210)) &
     &                +     speccomb1                                   &
     &                * (fac001*absa(ig,id001) + fac011*absa(ig,id011)  &
     &                +  fac101*absa(ig,id101) + fac111*absa(ig,id111)  &
     &                +  fac201*absa(ig,id201) + fac211*absa(ig,id211)) &
     &                + tauself + taufor + adjcolco2*absco2             &
     &                + colamt(k,7)*absco
 
          fracs(ns13+ig,k) = fracrefa(ig,jpl) + fpl                     &
     &                     * (fracrefa(ig,jplp) - fracrefa(ig,jpl))
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        indm = indminor(k)
        indmp = indm + 1
 
        do ig = 1, ng13
          abso3 = kb_mo3(ig,indm) + minorfrac(k)                        &
     &          * (kb_mo3(ig,indmp) - kb_mo3(ig,indm))
 
          taug(ns13+ig,k) = colamt(k,3)*abso3
 
          fracs(ns13+ig,k) =  fracrefb(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb13
! ----------------------------------
 
! ----------------------------------
      subroutine taugb14
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 14:  2250-2380 cm-1 (low - co2; high - co2)                 !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb14
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &       ig
 
      real (kind=kind_phys) :: tauself, taufor
!
!===> ...  begin here
!
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(14) + 1
        ind1 = ( jp(k)   *5 + (jt1(k)-1)) * nspa(14) + 1
 
        inds = indself(k)
        indf = indfor(k)
        ind0p = ind0 + 1
        ind1p = ind1 + 1
        indsp = inds + 1
        indfp = indf + 1
 
        do ig = 1, ng14
          tauself = selffac(k) * (selfref(ig,inds) + selffrac(k)        &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
 
          taug(ns14+ig,k) = colamt(k,2)                                 &
     &            * (fac00(k)*absa(ig,ind0) + fac10(k)*absa(ig,ind0p)   &
     &            +  fac01(k)*absa(ig,ind1) + fac11(k)*absa(ig,ind1p))  &
     &            + tauself + taufor
 
          fracs(ns14+ig,k) = fracrefa(ig)
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(14) + 1
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(14) + 1
 
        ind0p = ind0 + 1
        ind1p = ind1 + 1
 
        do ig = 1, ng14
          taug(ns14+ig,k) = colamt(k,2)                                 &
     &             * (fac00(k)*absb(ig,ind0) + fac10(k)*absb(ig,ind0p)  &
     &             +  fac01(k)*absb(ig,ind1) + fac11(k)*absb(ig,ind1p))
 
          fracs(ns14+ig,k) = fracrefb(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb14
! ----------------------------------
 
! ----------------------------------
      subroutine taugb15
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 15:  2380-2600 cm-1 (low - n2o,co2; low minor - n2)         !
!                              (high - nothing)                        !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb15
 
!  ---  locals:
      integer :: k, ind0, ind1, inds, indsp, indf, indfp, indm, indmp,  &
     &       id000, id010, id100, id110, id200, id210, jpl, jplp,       &
     &       id001, id011, id101, id111, id201, id211, jmn2, jmn2p,     &
     &       ig, js, js1
 
      real (kind=kind_phys) :: scalen2, tauself, taufor,                &
     &       speccomb,       specparm,       specmult,       fs,        &
     &       speccomb1,      specparm1,      specmult1,      fs1,       &
     &       speccomb_mn2,   specparm_mn2,   specmult_mn2,   fmn2,      &
     &       speccomb_planck,specparm_planck,specmult_planck,fpl,       &
     &       refrat_planck_a, refrat_m_a, n2m1, n2m2, taun2,            &
     &       fac000, fac100, fac200, fac010, fac110, fac210,            &
     &       fac001, fac101, fac201, fac011, fac111, fac211,            &
     &       p0, p40, fk00, fk10, fk20, p1, p41, fk01, fk11, fk21
!
!===> ...  begin here
!
!  --- ...  minor gas mapping level :
!     lower - nitrogen continuum, P = 1053., T = 294.
 
!  --- ...  calculate reference ratio to be used in calculation of Planck
!           fraction in lower atmosphere.
 
      refrat_planck_a = chi_mls(4,1)/chi_mls(2,1)      ! P = 1053. mb (Level 1)
      refrat_m_a = chi_mls(4,1)/chi_mls(2,1)           ! P = 1053. mb
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        speccomb = colamt(k,4) + rfrate(k,5,1)*colamt(k,2)
        specparm = colamt(k,4) / speccomb
        specmult = 8.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(15) + js
 
        speccomb1 = colamt(k,4) + rfrate(k,5,2)*colamt(k,2)
        specparm1 = colamt(k,4) / speccomb1
        specmult1 = 8.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = (jp(k)*5 + (jt1(k)-1)) * nspa(15) + js1
 
        speccomb_mn2 = colamt(k,4) + refrat_m_a*colamt(k,2)
        specparm_mn2 = colamt(k,4) / speccomb_mn2
        specmult_mn2 = 8.0 * min(specparm_mn2, oneminus)
        jmn2 = 1 + int(specmult_mn2)
        fmn2 = mod(specmult_mn2, f_one)
 
        speccomb_planck = colamt(k,4) + refrat_planck_a*colamt(k,2)
        specparm_planck = colamt(k,4) / speccomb_planck
        specmult_planck = 8.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
 
        scalen2 = colbrd(k) * scaleminor(k)
 
        inds = indself(k)
        indf = indfor(k)
        indm = indminor(k)
        indsp = inds + 1
        indfp = indf + 1
        indmp = indm + 1
        jplp  = jpl  + 1
        jmn2p = jmn2 + 1
 
        if (specparm < 0.125) then
          p0 = fs - f_one
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0 + 2
          id210 = ind0 +11
        elseif (specparm > 0.875) then
          p0 = -fs
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0 + 1
          id010 = ind0 +10
          id100 = ind0
          id110 = ind0 + 9
          id200 = ind0 - 1
          id210 = ind0 + 8
        else
          fk00 = f_one - fs
          fk10 = fs
          fk20 = f_zero
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0
          id210 = ind0
        endif
 
        fac000 = fk00 * fac00(k)
        fac100 = fk10 * fac00(k)
        fac200 = fk20 * fac00(k)
        fac010 = fk00 * fac10(k)
        fac110 = fk10 * fac10(k)
        fac210 = fk20 * fac10(k)
 
        if (specparm1 < 0.125) then
          p1 = fs1 - f_one
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1 + 2
          id211 = ind1 +11
        elseif (specparm1 > 0.875) then
          p1 = -fs1
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1 + 1
          id011 = ind1 +10
          id101 = ind1
          id111 = ind1 + 9
          id201 = ind1 - 1
          id211 = ind1 + 8
        else
          fk01 = f_one - fs1
          fk11 = fs1
          fk21 = f_zero
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1
          id211 = ind1
        endif
 
        fac001 = fk01 * fac01(k)
        fac101 = fk11 * fac01(k)
        fac201 = fk21 * fac01(k)
        fac011 = fk01 * fac11(k)
        fac111 = fk11 * fac11(k)
        fac211 = fk21 * fac11(k)
 
        do ig = 1, ng15
          tauself = selffac(k)* (selfref(ig,inds) + selffrac(k)         &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
          n2m1    = ka_mn2(ig,jmn2,indm) + fmn2                         &
     &            * (ka_mn2(ig,jmn2p,indm) - ka_mn2(ig,jmn2,indm))
          n2m2    = ka_mn2(ig,jmn2,indmp) + fmn2                        &
     &            * (ka_mn2(ig,jmn2p,indmp) - ka_mn2(ig,jmn2,indmp))
          taun2   = scalen2 * (n2m1 + minorfrac(k) * (n2m2 - n2m1))
 
          taug(ns15+ig,k) = speccomb                                    &
     &                * (fac000*absa(ig,id000) + fac010*absa(ig,id010)  &
     &                +  fac100*absa(ig,id100) + fac110*absa(ig,id110)  &
     &                +  fac200*absa(ig,id200) + fac210*absa(ig,id210)) &
     &                +     speccomb1                                   &
     &                * (fac001*absa(ig,id001) + fac011*absa(ig,id011)  &
     &                +  fac101*absa(ig,id101) + fac111*absa(ig,id111)  &
     &                +  fac201*absa(ig,id201) + fac211*absa(ig,id211)) &
     &                + tauself + taufor + taun2
 
          fracs(ns15+ig,k) = fracrefa(ig,jpl) + fpl                     &
     &                     * (fracrefa(ig,jplp) - fracrefa(ig,jpl))
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        do ig = 1, ng15
          taug(ns15+ig,k) = f_zero
 
          fracs(ns15+ig,k) = f_zero
        enddo
      enddo
 
! ..................................
      end subroutine taugb15
! ----------------------------------
 
! ----------------------------------
      subroutine taugb16
! ..................................
 
!  ------------------------------------------------------------------  !
!     band 16:  2600-3250 cm-1 (low key- h2o,ch4; high key - ch4)      !
!  ------------------------------------------------------------------  !
 
      use module_radlw_kgb16
 
!  ---  locals:
      integer :: k, ind0, ind0p, ind1, ind1p, inds, indsp, indf, indfp, &
     &       id000, id010, id100, id110, id200, id210, jpl, jplp,       &
     &       id001, id011, id101, id111, id201, id211, ig, js, js1
 
      real (kind=kind_phys) :: tauself, taufor, refrat_planck_a,        &
     &       speccomb,       specparm,       specmult,       fs,        &
     &       speccomb1,      specparm1,      specmult1,      fs1,       &
     &       speccomb_planck,specparm_planck,specmult_planck,fpl,       &
     &       fac000, fac100, fac200, fac010, fac110, fac210,            &
     &       fac001, fac101, fac201, fac011, fac111, fac211,            &
     &       p0, p40, fk00, fk10, fk20, p1, p41, fk01, fk11, fk21
!
!===> ...  begin here
!
!  --- ...  calculate reference ratio to be used in calculation of Planck
!           fraction in lower atmosphere.
 
      refrat_planck_a = chi_mls(1,6)/chi_mls(6,6)        ! P = 387. mb (Level 6)
 
!  --- ...  lower atmosphere loop
 
      do k = 1, laytrop
        speccomb = colamt(k,1) + rfrate(k,4,1)*colamt(k,5)
        specparm = colamt(k,1) / speccomb
        specmult = 8.0 * min(specparm, oneminus)
        js = 1 + int(specmult)
        fs = mod(specmult, f_one)
        ind0 = ((jp(k)-1)*5 + (jt(k)-1)) * nspa(16) + js
 
        speccomb1 = colamt(k,1) + rfrate(k,4,2)*colamt(k,5)
        specparm1 = colamt(k,1) / speccomb1
        specmult1 = 8.0 * min(specparm1, oneminus)
        js1 = 1 + int(specmult1)
        fs1 = mod(specmult1, f_one)
        ind1 = (jp(k)*5 + (jt1(k)-1)) * nspa(16) + js1
 
        speccomb_planck = colamt(k,1) + refrat_planck_a*colamt(k,5)
        specparm_planck = colamt(k,1) / speccomb_planck
        specmult_planck = 8.0 * min(specparm_planck, oneminus)
        jpl = 1 + int(specmult_planck)
        fpl = mod(specmult_planck, f_one)
 
        inds = indself(k)
        indf = indfor(k)
        indsp = inds + 1
        indfp = indf + 1
        jplp  = jpl  + 1
 
        if (specparm < 0.125) then
          p0 = fs - f_one
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0 + 2
          id210 = ind0 +11
        elseif (specparm > 0.875) then
          p0 = -fs
          p40 = p0**4
          fk00 = p40
          fk10 = f_one - p0 - 2.0*p40
          fk20 = p0 + p40
 
          id000 = ind0 + 1
          id010 = ind0 +10
          id100 = ind0
          id110 = ind0 + 9
          id200 = ind0 - 1
          id210 = ind0 + 8
        else
          fk00 = f_one - fs
          fk10 = fs
          fk20 = f_zero
 
          id000 = ind0
          id010 = ind0 + 9
          id100 = ind0 + 1
          id110 = ind0 +10
          id200 = ind0
          id210 = ind0
        endif
 
        fac000 = fk00 * fac00(k)
        fac100 = fk10 * fac00(k)
        fac200 = fk20 * fac00(k)
        fac010 = fk00 * fac10(k)
        fac110 = fk10 * fac10(k)
        fac210 = fk20 * fac10(k)
 
        if (specparm1 < 0.125) then
          p1 = fs1 - f_one
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1 + 2
          id211 = ind1 +11
        elseif (specparm1 > 0.875) then
          p1 = -fs1
          p41 = p1**4
          fk01 = p41
          fk11 = f_one - p1 - 2.0*p41
          fk21 = p1 + p41
 
          id001 = ind1 + 1
          id011 = ind1 +10
          id101 = ind1
          id111 = ind1 + 9
          id201 = ind1 - 1
          id211 = ind1 + 8
        else
          fk01 = f_one - fs1
          fk11 = fs1
          fk21 = f_zero
 
          id001 = ind1
          id011 = ind1 + 9
          id101 = ind1 + 1
          id111 = ind1 +10
          id201 = ind1
          id211 = ind1
        endif
 
        fac001 = fk01 * fac01(k)
        fac101 = fk11 * fac01(k)
        fac201 = fk21 * fac01(k)
        fac011 = fk01 * fac11(k)
        fac111 = fk11 * fac11(k)
        fac211 = fk21 * fac11(k)
 
        do ig = 1, ng16
          tauself = selffac(k)* (selfref(ig,inds) + selffrac(k)         &
     &            * (selfref(ig,indsp) - selfref(ig,inds)))
          taufor  = forfac(k) * (forref(ig,indf) + forfrac(k)           &
     &            * (forref(ig,indfp) - forref(ig,indf)))
 
          taug(ns16+ig,k) = speccomb                                    &
     &                * (fac000*absa(ig,id000) + fac010*absa(ig,id010)  &
     &                +  fac100*absa(ig,id100) + fac110*absa(ig,id110)  &
     &                +  fac200*absa(ig,id200) + fac210*absa(ig,id210)) &
     &                +     speccomb1                                   &
     &                * (fac001*absa(ig,id001) + fac011*absa(ig,id011)  &
     &                +  fac101*absa(ig,id101) + fac111*absa(ig,id111)  &
     &                +  fac201*absa(ig,id201) + fac211*absa(ig,id211)) &
     &                + tauself + taufor
 
          fracs(ns16+ig,k) = fracrefa(ig,jpl) + fpl                     &
     &                     * (fracrefa(ig,jplp) - fracrefa(ig,jpl))
        enddo
      enddo
 
!  --- ...  upper atmosphere loop
 
      do k = laytrop+1, nlay
        ind0 = ((jp(k)-13)*5 + (jt(k)-1)) * nspb(16) + 1
        ind1 = ((jp(k)-12)*5 + (jt1(k)-1)) * nspb(16) + 1
 
        ind0p = ind0 + 1
        ind1p = ind1 + 1
 
        do ig = 1, ng16
          taug(ns16+ig,k) = colamt(k,5)                                 &
     &           * (fac00(k)*absb(ig,ind0) + fac10(k)*absb(ig,ind0p)    &
     &           +  fac01(k)*absb(ig,ind1) + fac11(k)*absb(ig,ind1p))
 
          fracs(ns16+ig,k) = fracrefb(ig)
        enddo
      enddo
 
! ..................................
      end subroutine taugb16
! ----------------------------------
 
! ..................................
      end subroutine taumol
 
! ------------------------------------------------------------------------------
      subroutine cldprmc(nlayers, inflag, iceflag, liqflag, cldfmc,     &
     &  ciwpmc, clwpmc, cswpmc, reicmc, relqmc, resnmc, ncbands, taucmc, errmsg, errflg)
! ------------------------------------------------------------------------------
 
! Purpose:  Compute the cloud optical depth(s) for each cloudy layer.
 
! ------- Input -------
 
      integer(kind=im), intent(in) :: nlayers         ! total number of layers
      integer(kind=im), intent(in) :: inflag          ! see definitions
      integer(kind=im), intent(in) :: iceflag         ! see definitions
      integer(kind=im), intent(in) :: liqflag         ! see definitions
 
      real(kind=rb), intent(in) :: cldfmc(:,:)        ! cloud fraction [mcica]
                                                      !    Dimensions: (ngptlw,nlayers)
      real(kind=rb), intent(in) :: ciwpmc(:,:)        ! cloud ice water path [mcica]
                                                      !    Dimensions: (ngptlw,nlayers)
      real(kind=rb), intent(in) :: clwpmc(:,:)        ! cloud liquid water path [mcica]
                                                      !    Dimensions: (ngptlw,nlayers)
      real(kind=rb), intent(in) :: cswpmc(:,:)        ! cloud snow path [mcica]
                                                      !    Dimensions: (ngptlw,nlayers)
      real(kind=rb), intent(in) :: relqmc(:)          ! liquid particle effective radius (microns)
                                                      !    Dimensions: (nlayers)
      real(kind=rb), intent(in) :: reicmc(:)          ! ice particle effective radius (microns)
                                                      !    Dimensions: (nlayers)
      real(kind=rb), intent(in) :: resnmc(:)          ! snow particle effective radius (microns)
                                                      !    Dimensions: (nlayers)
                                                      ! specific definition of reicmc depends on setting of iceflag:
                                                      ! iceflag = 0: ice effective radius, r_ec, (Ebert and Curry, 1992),
                                                      !              r_ec must be >= 10.0 microns
                                                      ! iceflag = 1: ice effective radius, r_ec, (Ebert and Curry, 1992),
                                                      !              r_ec range is limited to 13.0 to 130.0 microns
                                                      ! iceflag = 2: ice effective radius, r_k, (Key, Streamer Ref. Manual, 1996)
                                                      !              r_k range is limited to 5.0 to 131.0 microns
                                                      ! iceflag = 3: generalized effective size, dge, (Fu, 1996),
                                                      !              dge range is limited to 5.0 to 140.0 microns
                                                      !              [dge = 1.0315 * r_ec]
 
! ------- Output -------
 
      integer(kind=im), intent(out)   :: ncbands      ! number of cloud spectral bands
      real(kind=rb),    intent(inout) :: taucmc(:,:)  ! cloud optical depth [mcica]
                                                      !    Dimensions: (ngptlw,nlayers)
      character(len=*), intent(inout) :: errmsg
      integer,          intent(inout) :: errflg
 
! ------- Local -------
 
      integer(kind=im) :: lay                         ! Layer index
      integer(kind=im) :: ib                          ! spectral band index
      integer(kind=im) :: ig                          ! g-point interval index
      integer(kind=im) :: index                                                                                     
      integer(kind=im) :: icb(nbands)                                                                               
      real(kind=rb) , dimension(2) :: absice0
      real(kind=rb) , dimension(2,5) :: absice1
      real(kind=rb) , dimension(43,16) :: absice2
      real(kind=rb) , dimension(46,16) :: absice3
      real(kind=rb) :: absliq0
      real(kind=rb) , dimension(58,16) :: absliq1
                                                                                                                    
      real(kind=rb) :: abscoice(ngptlw)               ! ice absorption coefficients                                 
      real(kind=rb) :: abscoliq(ngptlw)               ! liquid absorption coefficients                              
      real(kind=rb) :: abscosno(ngptlw)               ! snow absorption coefficients                                
      real(kind=rb) :: cwp                            ! cloud water path                                            
      real(kind=rb) :: radice                         ! cloud ice effective size (microns)                          
      real(kind=rb) :: factor                         !                                                             
      real(kind=rb) :: fint                           !                                                             
      real(kind=rb) :: radliq                         ! cloud liquid droplet radius (microns)                       
      real(kind=rb) :: radsno                         ! cloud snow effective size (microns)                         
      real(kind=rb), parameter :: eps = 1.e-6_rb      ! epsilon                                                     
      real(kind=rb), parameter :: cldmin = 1.e-20_rb  ! minimum value for cloud quantities                          
                                                                                                                    
! ------- Definitions -------                                                                                       
                                                                                                                    
!     Explanation of the method for each value of INFLAG.  Values of                                                
!     0 or 1 for INFLAG do not distingish being liquid and ice clouds.                                              
!     INFLAG = 2 does distinguish between liquid and ice clouds, and                                                
!     requires further user input to specify the method to be used to                                               
!     compute the aborption due to each.                                                                            
!     INFLAG = 0:  For each cloudy layer, the cloud fraction and (gray)                                             
!                  optical depth are input.                                                                         
!     INFLAG = 1:  For each cloudy layer, the cloud fraction and cloud                                              
!                  water path (g/m2) are input.  The (gray) cloud optical                                           
!                  depth is computed as in CCM2.                                                                    
!     INFLAG = 2:  For each cloudy layer, the cloud fraction, cloud                                                 
!                  water path (g/m2), and cloud ice fraction are input.                                             
!       ICEFLAG = 0:  The ice effective radius (microns) is input and the                                           
!                     optical depths due to ice clouds are computed as in CCM3.                                     
!       ICEFLAG = 1:  The ice effective radius (microns) is input and the                                           
!                     optical depths due to ice clouds are computed as in                                           
!                     Ebert and Curry, JGR, 97, 3831-3836 (1992).  The                                              
!                     spectral regions in this work have been matched with                                          
!                     the spectral bands in RRTM to as great an extent                                              
!                     as possible:                                                                                  
!                     E&C 1      IB = 5      RRTM bands 9-16                                                        
!                     E&C 2      IB = 4      RRTM bands 6-8                                                         
!                     E&C 3      IB = 3      RRTM bands 3-5                                                         
!                     E&C 4      IB = 2      RRTM band 2                                                            
!                     E&C 5      IB = 1      RRTM band 1                                                            
!       ICEFLAG = 2:  The ice effective radius (microns) is input and the
!                     optical properties due to ice clouds are computed from
!                     the optical properties stored in the RT code,
!                     STREAMER v3.0 (Reference: Key. J., Streamer 
!                     User's Guide, Cooperative Institute for
!                     Meteorological Satellite Studies, 2001, 96 pp.).
!                     Valid range of values for re are between 5.0 and
!                     131.0 micron.
!       ICEFLAG = 3: The ice generalized effective size (dge) is input
!                    and the optical properties, are calculated as in
!                    Q. Fu, J. Climate, (1998). Q. Fu provided high resolution
!                    tables which were appropriately averaged for the
!                    bands in RRTM_LW.  Linear interpolation is used to
!                    get the coefficients from the stored tables.
!                    Valid range of values for dge are between 5.0 and
!                    140.0 micron.
!       LIQFLAG = 0:  The optical depths due to water clouds are computed as
!                     in CCM3.
!       LIQFLAG = 1:  The water droplet effective radius (microns) is input 
!                     and the optical depths due to water clouds are computed 
!                     as in Hu and Stamnes, J., Clim., 6, 728-742, (1993).
!                     The values for absorption coefficients appropriate for
!                     the spectral bands in RRTM have been obtained for a 
!                     range of effective radii by an averaging procedure 
!                     based on the work of J. Pinto (private communication).
!                     Linear interpolation is used to get the absorption 
!                     coefficients for the input effective radius.
 
      data icb /1,2,3,3,3,4,4,4,5, 5, 5, 5, 5, 5, 5, 5/
! Everything below is for INFLAG = 2.
 
! ABSICEn(J,IB) are the parameters needed to compute the liquid water 
! absorption coefficient in spectral region IB for ICEFLAG=n.  The units
! of ABSICEn(1,IB) are m2/g and ABSICEn(2,IB) has units (microns (m2/g)).
! For ICEFLAG = 0.
 
      absice0(:)= (/0.005_rb,  1.0_rb/)
 
! For ICEFLAG = 1.
      absice1(1,:) = (/0.0036_rb, 0.0068_rb, 0.0003_rb, 0.0016_rb,      &
     &                0.0020_rb/)
      absice1(2,:) = (/1.136_rb , 0.600_rb , 1.338_rb , 1.166_rb ,      &
     &                1.118_rb /)
 
! For ICEFLAG = 2.  In each band, the absorption
! coefficients are listed for a range of effective radii from 5.0
! to 131.0 microns in increments of 3.0 microns.
! Spherical Ice Particle Parameterization
! absorption units (abs coef/iwc): [(m^-1)/(g m^-3)]
      absice2(:,1) = (/ &
! band 1
       7.798999e-02_rb,6.340479e-02_rb,5.417973e-02_rb,4.766245e-02_rb,4.272663e-02_rb, &
       3.880939e-02_rb,3.559544e-02_rb,3.289241e-02_rb,3.057511e-02_rb,2.855800e-02_rb, &
       2.678022e-02_rb,2.519712e-02_rb,2.377505e-02_rb,2.248806e-02_rb,2.131578e-02_rb, &
       2.024194e-02_rb,1.925337e-02_rb,1.833926e-02_rb,1.749067e-02_rb,1.670007e-02_rb, &
       1.596113e-02_rb,1.526845e-02_rb,1.461739e-02_rb,1.400394e-02_rb,1.342462e-02_rb, &
       1.287639e-02_rb,1.235656e-02_rb,1.186279e-02_rb,1.139297e-02_rb,1.094524e-02_rb, &
       1.051794e-02_rb,1.010956e-02_rb,9.718755e-03_rb,9.344316e-03_rb,8.985139e-03_rb, &
       8.640223e-03_rb,8.308656e-03_rb,7.989606e-03_rb,7.682312e-03_rb,7.386076e-03_rb, &
       7.100255e-03_rb,6.824258e-03_rb,6.557540e-03_rb/)
      absice2(:,2) = (/ &
! band 2
       2.784879e-02_rb,2.709863e-02_rb,2.619165e-02_rb,2.529230e-02_rb,2.443225e-02_rb, &
       2.361575e-02_rb,2.284021e-02_rb,2.210150e-02_rb,2.139548e-02_rb,2.071840e-02_rb, &
       2.006702e-02_rb,1.943856e-02_rb,1.883064e-02_rb,1.824120e-02_rb,1.766849e-02_rb, &
       1.711099e-02_rb,1.656737e-02_rb,1.603647e-02_rb,1.551727e-02_rb,1.500886e-02_rb, &
       1.451045e-02_rb,1.402132e-02_rb,1.354084e-02_rb,1.306842e-02_rb,1.260355e-02_rb, &
       1.214575e-02_rb,1.169460e-02_rb,1.124971e-02_rb,1.081072e-02_rb,1.037731e-02_rb, &
       9.949167e-03_rb,9.526021e-03_rb,9.107615e-03_rb,8.693714e-03_rb,8.284096e-03_rb, &
       7.878558e-03_rb,7.476910e-03_rb,7.078974e-03_rb,6.684586e-03_rb,6.293589e-03_rb, &
       5.905839e-03_rb,5.521200e-03_rb,5.139543e-03_rb/)
      absice2(:,3) = (/ &
! band 3
       1.065397e-01_rb,8.005726e-02_rb,6.546428e-02_rb,5.589131e-02_rb,4.898681e-02_rb, &
       4.369932e-02_rb,3.947901e-02_rb,3.600676e-02_rb,3.308299e-02_rb,3.057561e-02_rb, &
       2.839325e-02_rb,2.647040e-02_rb,2.475872e-02_rb,2.322164e-02_rb,2.183091e-02_rb, &
       2.056430e-02_rb,1.940407e-02_rb,1.833586e-02_rb,1.734787e-02_rb,1.643034e-02_rb, &
       1.557512e-02_rb,1.477530e-02_rb,1.402501e-02_rb,1.331924e-02_rb,1.265364e-02_rb, &
       1.202445e-02_rb,1.142838e-02_rb,1.086257e-02_rb,1.032445e-02_rb,9.811791e-03_rb, &
       9.322587e-03_rb,8.855053e-03_rb,8.407591e-03_rb,7.978763e-03_rb,7.567273e-03_rb, &
       7.171949e-03_rb,6.791728e-03_rb,6.425642e-03_rb,6.072809e-03_rb,5.732424e-03_rb, &
       5.403748e-03_rb,5.086103e-03_rb,4.778865e-03_rb/)
      absice2(:,4) = (/ &
! band 4
       1.804566e-01_rb,1.168987e-01_rb,8.680442e-02_rb,6.910060e-02_rb,5.738174e-02_rb, &
       4.902332e-02_rb,4.274585e-02_rb,3.784923e-02_rb,3.391734e-02_rb,3.068690e-02_rb, &
       2.798301e-02_rb,2.568480e-02_rb,2.370600e-02_rb,2.198337e-02_rb,2.046940e-02_rb, &   
       1.912777e-02_rb,1.793016e-02_rb,1.685420e-02_rb,1.588193e-02_rb,1.499882e-02_rb, &   
       1.419293e-02_rb,1.345440e-02_rb,1.277496e-02_rb,1.214769e-02_rb,1.156669e-02_rb, &   
       1.102694e-02_rb,1.052412e-02_rb,1.005451e-02_rb,9.614854e-03_rb,9.202335e-03_rb, &   
       8.814470e-03_rb,8.449077e-03_rb,8.104223e-03_rb,7.778195e-03_rb,7.469466e-03_rb, &   
       7.176671e-03_rb,6.898588e-03_rb,6.634117e-03_rb,6.382264e-03_rb,6.142134e-03_rb, &   
       5.912913e-03_rb,5.693862e-03_rb,5.484308e-03_rb/)                                    
      absice2(:,5) = (/ &                                                                   
! band 5                                                                                    
       2.131806e-01_rb,1.311372e-01_rb,9.407171e-02_rb,7.299442e-02_rb,5.941273e-02_rb, &   
       4.994043e-02_rb,4.296242e-02_rb,3.761113e-02_rb,3.337910e-02_rb,2.994978e-02_rb, &   
       2.711556e-02_rb,2.473461e-02_rb,2.270681e-02_rb,2.095943e-02_rb,1.943839e-02_rb, &   
       1.810267e-02_rb,1.692057e-02_rb,1.586719e-02_rb,1.492275e-02_rb,1.407132e-02_rb, &   
       1.329989e-02_rb,1.259780e-02_rb,1.195618e-02_rb,1.136761e-02_rb,1.082583e-02_rb, &   
       1.032552e-02_rb,9.862158e-03_rb,9.431827e-03_rb,9.031157e-03_rb,8.657217e-03_rb, &   
       8.307449e-03_rb,7.979609e-03_rb,7.671724e-03_rb,7.382048e-03_rb,7.109032e-03_rb, &   
       6.851298e-03_rb,6.607615e-03_rb,6.376881e-03_rb,6.158105e-03_rb,5.950394e-03_rb, &   
       5.752942e-03_rb,5.565019e-03_rb,5.385963e-03_rb/)                                    
      absice2(:,6) = (/ &                                                                   
! band 6                                                                                    
       1.546177e-01_rb,1.039251e-01_rb,7.910347e-02_rb,6.412429e-02_rb,5.399997e-02_rb, &   
       4.664937e-02_rb,4.104237e-02_rb,3.660781e-02_rb,3.300218e-02_rb,3.000586e-02_rb, &   
       2.747148e-02_rb,2.529633e-02_rb,2.340647e-02_rb,2.174723e-02_rb,2.027731e-02_rb, &   
       1.896487e-02_rb,1.778492e-02_rb,1.671761e-02_rb,1.574692e-02_rb,1.485978e-02_rb, &   
       1.404543e-02_rb,1.329489e-02_rb,1.260066e-02_rb,1.195636e-02_rb,1.135657e-02_rb, &   
       1.079664e-02_rb,1.027257e-02_rb,9.780871e-03_rb,9.318505e-03_rb,8.882815e-03_rb, &   
       8.471458e-03_rb,8.082364e-03_rb,7.713696e-03_rb,7.363817e-03_rb,7.031264e-03_rb, &   
       6.714725e-03_rb,6.413021e-03_rb,6.125086e-03_rb,5.849958e-03_rb,5.586764e-03_rb, &   
       5.334707e-03_rb,5.093066e-03_rb,4.861179e-03_rb/)                                    
      absice2(:,7) = (/ &                                                                   
! band 7                                                                                    
       7.583404e-02_rb,6.181558e-02_rb,5.312027e-02_rb,4.696039e-02_rb,4.225986e-02_rb, &   
       3.849735e-02_rb,3.538340e-02_rb,3.274182e-02_rb,3.045798e-02_rb,2.845343e-02_rb, &   
       2.667231e-02_rb,2.507353e-02_rb,2.362606e-02_rb,2.230595e-02_rb,2.109435e-02_rb, &   
       1.997617e-02_rb,1.893916e-02_rb,1.797328e-02_rb,1.707016e-02_rb,1.622279e-02_rb, &   
       1.542523e-02_rb,1.467241e-02_rb,1.395997e-02_rb,1.328414e-02_rb,1.264164e-02_rb, &   
       1.202958e-02_rb,1.144544e-02_rb,1.088697e-02_rb,1.035218e-02_rb,9.839297e-03_rb, &   
       9.346733e-03_rb,8.873057e-03_rb,8.416980e-03_rb,7.977335e-03_rb,7.553066e-03_rb, &   
       7.143210e-03_rb,6.746888e-03_rb,6.363297e-03_rb,5.991700e-03_rb,5.631422e-03_rb, &   
       5.281840e-03_rb,4.942378e-03_rb,4.612505e-03_rb/)                                    
      absice2(:,8) = (/ &                                                                   
! band 8                                                                                    
       9.022185e-02_rb,6.922700e-02_rb,5.710674e-02_rb,4.898377e-02_rb,4.305946e-02_rb, &   
       3.849553e-02_rb,3.484183e-02_rb,3.183220e-02_rb,2.929794e-02_rb,2.712627e-02_rb, &   
       2.523856e-02_rb,2.357810e-02_rb,2.210286e-02_rb,2.078089e-02_rb,1.958747e-02_rb, &   
       1.850310e-02_rb,1.751218e-02_rb,1.660205e-02_rb,1.576232e-02_rb,1.498440e-02_rb, &   
       1.426107e-02_rb,1.358624e-02_rb,1.295474e-02_rb,1.236212e-02_rb,1.180456e-02_rb, &   
       1.127874e-02_rb,1.078175e-02_rb,1.031106e-02_rb,9.864433e-03_rb,9.439878e-03_rb, &   
       9.035637e-03_rb,8.650140e-03_rb,8.281981e-03_rb,7.929895e-03_rb,7.592746e-03_rb, &   
       7.269505e-03_rb,6.959238e-03_rb,6.661100e-03_rb,6.374317e-03_rb,6.098185e-03_rb, &   
       5.832059e-03_rb,5.575347e-03_rb,5.327504e-03_rb/)                                    
      absice2(:,9) = (/ &
! band 9
       1.294087e-01_rb,8.788217e-02_rb,6.728288e-02_rb,5.479720e-02_rb,4.635049e-02_rb, &
       4.022253e-02_rb,3.555576e-02_rb,3.187259e-02_rb,2.888498e-02_rb,2.640843e-02_rb, &
       2.431904e-02_rb,2.253038e-02_rb,2.098024e-02_rb,1.962267e-02_rb,1.842293e-02_rb, &
       1.735426e-02_rb,1.639571e-02_rb,1.553060e-02_rb,1.474552e-02_rb,1.402953e-02_rb, &
       1.337363e-02_rb,1.277033e-02_rb,1.221336e-02_rb,1.169741e-02_rb,1.121797e-02_rb, &
       1.077117e-02_rb,1.035369e-02_rb,9.962643e-03_rb,9.595509e-03_rb,9.250088e-03_rb, &
       8.924447e-03_rb,8.616876e-03_rb,8.325862e-03_rb,8.050057e-03_rb,7.788258e-03_rb, &
       7.539388e-03_rb,7.302478e-03_rb,7.076656e-03_rb,6.861134e-03_rb,6.655197e-03_rb, &
       6.458197e-03_rb,6.269543e-03_rb,6.088697e-03_rb/)
      absice2(:,10) = (/ &
! band 10
       1.593628e-01_rb,1.014552e-01_rb,7.458955e-02_rb,5.903571e-02_rb,4.887582e-02_rb, &
       4.171159e-02_rb,3.638480e-02_rb,3.226692e-02_rb,2.898717e-02_rb,2.631256e-02_rb, &
       2.408925e-02_rb,2.221156e-02_rb,2.060448e-02_rb,1.921325e-02_rb,1.799699e-02_rb, &
       1.692456e-02_rb,1.597177e-02_rb,1.511961e-02_rb,1.435289e-02_rb,1.365933e-02_rb, &
       1.302890e-02_rb,1.245334e-02_rb,1.192576e-02_rb,1.144037e-02_rb,1.099230e-02_rb, &   
       1.057739e-02_rb,1.019208e-02_rb,9.833302e-03_rb,9.498395e-03_rb,9.185047e-03_rb, &   
       8.891237e-03_rb,8.615185e-03_rb,8.355325e-03_rb,8.110267e-03_rb,7.878778e-03_rb, &   
       7.659759e-03_rb,7.452224e-03_rb,7.255291e-03_rb,7.068166e-03_rb,6.890130e-03_rb, &   
       6.720536e-03_rb,6.558794e-03_rb,6.404371e-03_rb/)                                    
      absice2(:,11) = (/ &                                                                  
! band 11                                                                                   
       1.656227e-01_rb,1.032129e-01_rb,7.487359e-02_rb,5.871431e-02_rb,4.828355e-02_rb, &   
       4.099989e-02_rb,3.562924e-02_rb,3.150755e-02_rb,2.824593e-02_rb,2.560156e-02_rb, &   
       2.341503e-02_rb,2.157740e-02_rb,2.001169e-02_rb,1.866199e-02_rb,1.748669e-02_rb, &   
       1.645421e-02_rb,1.554015e-02_rb,1.472535e-02_rb,1.399457e-02_rb,1.333553e-02_rb, &   
       1.273821e-02_rb,1.219440e-02_rb,1.169725e-02_rb,1.124104e-02_rb,1.082096e-02_rb, &   
       1.043290e-02_rb,1.007336e-02_rb,9.739338e-03_rb,9.428223e-03_rb,9.137756e-03_rb, &   
       8.865964e-03_rb,8.611115e-03_rb,8.371686e-03_rb,8.146330e-03_rb,7.933852e-03_rb, &   
       7.733187e-03_rb,7.543386e-03_rb,7.363597e-03_rb,7.193056e-03_rb,7.031072e-03_rb, &   
       6.877024e-03_rb,6.730348e-03_rb,6.590531e-03_rb/)                                    
      absice2(:,12) = (/ &                                                                  
! band 12                                                                                   
       9.194591e-02_rb,6.446867e-02_rb,4.962034e-02_rb,4.042061e-02_rb,3.418456e-02_rb, &   
       2.968856e-02_rb,2.629900e-02_rb,2.365572e-02_rb,2.153915e-02_rb,1.980791e-02_rb, &   
       1.836689e-02_rb,1.714979e-02_rb,1.610900e-02_rb,1.520946e-02_rb,1.442476e-02_rb, &   
       1.373468e-02_rb,1.312345e-02_rb,1.257858e-02_rb,1.209010e-02_rb,1.164990e-02_rb, &   
       1.125136e-02_rb,1.088901e-02_rb,1.055827e-02_rb,1.025531e-02_rb,9.976896e-03_rb, &   
       9.720255e-03_rb,9.483022e-03_rb,9.263160e-03_rb,9.058902e-03_rb,8.868710e-03_rb, &   
       8.691240e-03_rb,8.525312e-03_rb,8.369886e-03_rb,8.224042e-03_rb,8.086961e-03_rb, &   
       7.957917e-03_rb,7.836258e-03_rb,7.721400e-03_rb,7.612821e-03_rb,7.510045e-03_rb, &   
       7.412648e-03_rb,7.320242e-03_rb,7.232476e-03_rb/)           
      absice2(:,13) = (/ &
! band 13                                                                                   
       1.437021e-01_rb,8.872535e-02_rb,6.392420e-02_rb,4.991833e-02_rb,4.096790e-02_rb, &   
       3.477881e-02_rb,3.025782e-02_rb,2.681909e-02_rb,2.412102e-02_rb,2.195132e-02_rb, &   
       2.017124e-02_rb,1.868641e-02_rb,1.743044e-02_rb,1.635529e-02_rb,1.542540e-02_rb, &   
       1.461388e-02_rb,1.390003e-02_rb,1.326766e-02_rb,1.270395e-02_rb,1.219860e-02_rb, &   
       1.174326e-02_rb,1.133107e-02_rb,1.095637e-02_rb,1.061442e-02_rb,1.030126e-02_rb, &   
       1.001352e-02_rb,9.748340e-03_rb,9.503256e-03_rb,9.276155e-03_rb,9.065205e-03_rb, &   
       8.868808e-03_rb,8.685571e-03_rb,8.514268e-03_rb,8.353820e-03_rb,8.203272e-03_rb, &   
       8.061776e-03_rb,7.928578e-03_rb,7.803001e-03_rb,7.684443e-03_rb,7.572358e-03_rb, &   
       7.466258e-03_rb,7.365701e-03_rb,7.270286e-03_rb/)                                    
      absice2(:,14) = (/ &                                                                  
! band 14                                                                                   
       1.288870e-01_rb,8.160295e-02_rb,5.964745e-02_rb,4.703790e-02_rb,3.888637e-02_rb, &   
       3.320115e-02_rb,2.902017e-02_rb,2.582259e-02_rb,2.330224e-02_rb,2.126754e-02_rb, &   
       1.959258e-02_rb,1.819130e-02_rb,1.700289e-02_rb,1.598320e-02_rb,1.509942e-02_rb, &   
       1.432666e-02_rb,1.364572e-02_rb,1.304156e-02_rb,1.250220e-02_rb,1.201803e-02_rb, &   
       1.158123e-02_rb,1.118537e-02_rb,1.082513e-02_rb,1.049605e-02_rb,1.019440e-02_rb, &   
       9.916989e-03_rb,9.661116e-03_rb,9.424457e-03_rb,9.205005e-03_rb,9.001022e-03_rb, &   
       8.810992e-03_rb,8.633588e-03_rb,8.467646e-03_rb,8.312137e-03_rb,8.166151e-03_rb, &   
       8.028878e-03_rb,7.899597e-03_rb,7.777663e-03_rb,7.662498e-03_rb,7.553581e-03_rb, &   
       7.450444e-03_rb,7.352662e-03_rb,7.259851e-03_rb/)                                    
      absice2(:,15) = (/ &                                                                  
! band 15                                                                                   
       8.254229e-02_rb,5.808787e-02_rb,4.492166e-02_rb,3.675028e-02_rb,3.119623e-02_rb, &   
       2.718045e-02_rb,2.414450e-02_rb,2.177073e-02_rb,1.986526e-02_rb,1.830306e-02_rb, &   
       1.699991e-02_rb,1.589698e-02_rb,1.495199e-02_rb,1.413374e-02_rb,1.341870e-02_rb, &   
       1.278883e-02_rb,1.223002e-02_rb,1.173114e-02_rb,1.128322e-02_rb,1.087900e-02_rb, &   
       1.051254e-02_rb,1.017890e-02_rb,9.873991e-03_rb,9.594347e-03_rb,9.337044e-03_rb, &   
       9.099589e-03_rb,8.879842e-03_rb,8.675960e-03_rb,8.486341e-03_rb,8.309594e-03_rb, &   
       8.144500e-03_rb,7.989986e-03_rb,7.845109e-03_rb,7.709031e-03_rb,7.581007e-03_rb, &   
       7.460376e-03_rb,7.346544e-03_rb,7.238978e-03_rb,7.137201e-03_rb,7.040780e-03_rb, &   
       6.949325e-03_rb,6.862483e-03_rb,6.779931e-03_rb/)                                    
      absice2(:,16) = (/ &                                                                  
! band 16                                                                                   
       1.382062e-01_rb,8.643227e-02_rb,6.282935e-02_rb,4.934783e-02_rb,4.063891e-02_rb, &   
       3.455591e-02_rb,3.007059e-02_rb,2.662897e-02_rb,2.390631e-02_rb,2.169972e-02_rb, &   
       1.987596e-02_rb,1.834393e-02_rb,1.703924e-02_rb,1.591513e-02_rb,1.493679e-02_rb, &   
       1.407780e-02_rb,1.331775e-02_rb,1.264061e-02_rb,1.203364e-02_rb,1.148655e-02_rb, &   
       1.099099e-02_rb,1.054006e-02_rb,1.012807e-02_rb,9.750215e-03_rb,9.402477e-03_rb, &   
       9.081428e-03_rb,8.784143e-03_rb,8.508107e-03_rb,8.251146e-03_rb,8.011373e-03_rb, &   
       7.787140e-03_rb,7.577002e-03_rb,7.379687e-03_rb,7.194071e-03_rb,7.019158e-03_rb, &   
       6.854061e-03_rb,6.697986e-03_rb,6.550224e-03_rb,6.410138e-03_rb,6.277153e-03_rb, &   
       6.150751e-03_rb,6.030462e-03_rb,5.915860e-03_rb/)                                    
                                                                                           
! ICEFLAG = 3; Fu parameterization. Particle size 5 - 140 micron in 
! increments of 3 microns.
! units = m2/g
! Hexagonal Ice Particle Parameterization
! absorption units (abs coef/iwc): [(m^-1)/(g m^-3)]
      absice3(:,1) = (/ &
! band 1
       3.110649e-03_rb,4.666352e-02_rb,6.606447e-02_rb,6.531678e-02_rb,6.012598e-02_rb, &
       5.437494e-02_rb,4.906411e-02_rb,4.441146e-02_rb,4.040585e-02_rb,3.697334e-02_rb, &
       3.403027e-02_rb,3.149979e-02_rb,2.931596e-02_rb,2.742365e-02_rb,2.577721e-02_rb, &
       2.433888e-02_rb,2.307732e-02_rb,2.196644e-02_rb,2.098437e-02_rb,2.011264e-02_rb, &
       1.933561e-02_rb,1.863992e-02_rb,1.801407e-02_rb,1.744812e-02_rb,1.693346e-02_rb, &
       1.646252e-02_rb,1.602866e-02_rb,1.562600e-02_rb,1.524933e-02_rb,1.489399e-02_rb, &
       1.455580e-02_rb,1.423098e-02_rb,1.391612e-02_rb,1.360812e-02_rb,1.330413e-02_rb, &
       1.300156e-02_rb,1.269801e-02_rb,1.239127e-02_rb,1.207928e-02_rb,1.176014e-02_rb, &
       1.143204e-02_rb,1.109334e-02_rb,1.074243e-02_rb,1.037786e-02_rb,9.998198e-03_rb, &
       9.602126e-03_rb/)
      absice3(:,2) = (/ &
! band 2
       3.984966e-04_rb,1.681097e-02_rb,2.627680e-02_rb,2.767465e-02_rb,2.700722e-02_rb, &
       2.579180e-02_rb,2.448677e-02_rb,2.323890e-02_rb,2.209096e-02_rb,2.104882e-02_rb, &
       2.010547e-02_rb,1.925003e-02_rb,1.847128e-02_rb,1.775883e-02_rb,1.710358e-02_rb, &
       1.649769e-02_rb,1.593449e-02_rb,1.540829e-02_rb,1.491429e-02_rb,1.444837e-02_rb, &
       1.400704e-02_rb,1.358729e-02_rb,1.318654e-02_rb,1.280258e-02_rb,1.243346e-02_rb, &
       1.207750e-02_rb,1.173325e-02_rb,1.139941e-02_rb,1.107487e-02_rb,1.075861e-02_rb, &
       1.044975e-02_rb,1.014753e-02_rb,9.851229e-03_rb,9.560240e-03_rb,9.274003e-03_rb, &
       8.992020e-03_rb,8.713845e-03_rb,8.439074e-03_rb,8.167346e-03_rb,7.898331e-03_rb, &
       7.631734e-03_rb,7.367286e-03_rb,7.104742e-03_rb,6.843882e-03_rb,6.584504e-03_rb, &
       6.326424e-03_rb/)
      absice3(:,3) = (/ &
! band 3
       6.933163e-02_rb,8.540475e-02_rb,7.701816e-02_rb,6.771158e-02_rb,5.986953e-02_rb, &
       5.348120e-02_rb,4.824962e-02_rb,4.390563e-02_rb,4.024411e-02_rb,3.711404e-02_rb, &
       3.440426e-02_rb,3.203200e-02_rb,2.993478e-02_rb,2.806474e-02_rb,2.638464e-02_rb, &
       2.486516e-02_rb,2.348288e-02_rb,2.221890e-02_rb,2.105780e-02_rb,1.998687e-02_rb, &
       1.899552e-02_rb,1.807490e-02_rb,1.721750e-02_rb,1.641693e-02_rb,1.566773e-02_rb, &
       1.496515e-02_rb,1.430509e-02_rb,1.368398e-02_rb,1.309865e-02_rb,1.254634e-02_rb, &
       1.202456e-02_rb,1.153114e-02_rb,1.106409e-02_rb,1.062166e-02_rb,1.020224e-02_rb, &
       9.804381e-03_rb,9.426771e-03_rb,9.068205e-03_rb,8.727578e-03_rb,8.403876e-03_rb, &
       8.096160e-03_rb,7.803564e-03_rb,7.525281e-03_rb,7.260560e-03_rb,7.008697e-03_rb, &
       6.769036e-03_rb/)
      absice3(:,4) = (/ &
! band 4
       1.765735e-01_rb,1.382700e-01_rb,1.095129e-01_rb,8.987475e-02_rb,7.591185e-02_rb, &
       6.554169e-02_rb,5.755500e-02_rb,5.122083e-02_rb,4.607610e-02_rb,4.181475e-02_rb, &
       3.822697e-02_rb,3.516432e-02_rb,3.251897e-02_rb,3.021073e-02_rb,2.817876e-02_rb, &
       2.637607e-02_rb,2.476582e-02_rb,2.331871e-02_rb,2.201113e-02_rb,2.082388e-02_rb, &
       1.974115e-02_rb,1.874983e-02_rb,1.783894e-02_rb,1.699922e-02_rb,1.622280e-02_rb, &
       1.550296e-02_rb,1.483390e-02_rb,1.421064e-02_rb,1.362880e-02_rb,1.308460e-02_rb, &
       1.257468e-02_rb,1.209611e-02_rb,1.164628e-02_rb,1.122287e-02_rb,1.082381e-02_rb, &
       1.044725e-02_rb,1.009154e-02_rb,9.755166e-03_rb,9.436783e-03_rb,9.135163e-03_rb, &
       8.849193e-03_rb,8.577856e-03_rb,8.320225e-03_rb,8.075451e-03_rb,7.842755e-03_rb, &
       7.621418e-03_rb/)
      absice3(:,5) = (/ &
! band 5
       2.339673e-01_rb,1.692124e-01_rb,1.291656e-01_rb,1.033837e-01_rb,8.562949e-02_rb, &
       7.273526e-02_rb,6.298262e-02_rb,5.537015e-02_rb,4.927787e-02_rb,4.430246e-02_rb, &
       4.017061e-02_rb,3.669072e-02_rb,3.372455e-02_rb,3.116995e-02_rb,2.894977e-02_rb, &
       2.700471e-02_rb,2.528842e-02_rb,2.376420e-02_rb,2.240256e-02_rb,2.117959e-02_rb, &
       2.007567e-02_rb,1.907456e-02_rb,1.816271e-02_rb,1.732874e-02_rb,1.656300e-02_rb, &
       1.585725e-02_rb,1.520445e-02_rb,1.459852e-02_rb,1.403419e-02_rb,1.350689e-02_rb, &
       1.301260e-02_rb,1.254781e-02_rb,1.210941e-02_rb,1.169468e-02_rb,1.130118e-02_rb, &
       1.092675e-02_rb,1.056945e-02_rb,1.022757e-02_rb,9.899560e-03_rb,9.584021e-03_rb, &
       9.279705e-03_rb,8.985479e-03_rb,8.700322e-03_rb,8.423306e-03_rb,8.153590e-03_rb, &
       7.890412e-03_rb/)                                                             
      absice3(:,6) = (/ &                                                            
! band 6                                                                             
       1.145369e-01_rb,1.174566e-01_rb,9.917866e-02_rb,8.332990e-02_rb,7.104263e-02_rb, &
       6.153370e-02_rb,5.405472e-02_rb,4.806281e-02_rb,4.317918e-02_rb,3.913795e-02_rb, &
       3.574916e-02_rb,3.287437e-02_rb,3.041067e-02_rb,2.828017e-02_rb,2.642292e-02_rb, &
       2.479206e-02_rb,2.335051e-02_rb,2.206851e-02_rb,2.092195e-02_rb,1.989108e-02_rb, &
       1.895958e-02_rb,1.811385e-02_rb,1.734245e-02_rb,1.663573e-02_rb,1.598545e-02_rb, &
       1.538456e-02_rb,1.482700e-02_rb,1.430750e-02_rb,1.382150e-02_rb,1.336499e-02_rb, &
       1.293447e-02_rb,1.252685e-02_rb,1.213939e-02_rb,1.176968e-02_rb,1.141555e-02_rb, &
       1.107508e-02_rb,1.074655e-02_rb,1.042839e-02_rb,1.011923e-02_rb,9.817799e-03_rb, &
       9.522962e-03_rb,9.233688e-03_rb,8.949041e-03_rb,8.668171e-03_rb,8.390301e-03_rb, &
       8.114723e-03_rb/)                                                             
      absice3(:,7) = (/ &                                                            
! band 7                                                                             
       1.222345e-02_rb,5.344230e-02_rb,5.523465e-02_rb,5.128759e-02_rb,4.676925e-02_rb, &
       4.266150e-02_rb,3.910561e-02_rb,3.605479e-02_rb,3.342843e-02_rb,3.115052e-02_rb, &
       2.915776e-02_rb,2.739935e-02_rb,2.583499e-02_rb,2.443266e-02_rb,2.316681e-02_rb, &
       2.201687e-02_rb,2.096619e-02_rb,2.000112e-02_rb,1.911044e-02_rb,1.828481e-02_rb, &
       1.751641e-02_rb,1.679866e-02_rb,1.612598e-02_rb,1.549360e-02_rb,1.489742e-02_rb, &
       1.433392e-02_rb,1.380002e-02_rb,1.329305e-02_rb,1.281068e-02_rb,1.235084e-02_rb, &
       1.191172e-02_rb,1.149171e-02_rb,1.108936e-02_rb,1.070341e-02_rb,1.033271e-02_rb, &
       9.976220e-03_rb,9.633021e-03_rb,9.302273e-03_rb,8.983216e-03_rb,8.675161e-03_rb, &
       8.377478e-03_rb,8.089595e-03_rb,7.810986e-03_rb,7.541170e-03_rb,7.279706e-03_rb, &
       7.026186e-03_rb/)                                                             
      absice3(:,8) = (/ &                                                            
! band 8                                                                             
       6.711058e-02_rb,6.918198e-02_rb,6.127484e-02_rb,5.411944e-02_rb,4.836902e-02_rb, &
       4.375293e-02_rb,3.998077e-02_rb,3.683587e-02_rb,3.416508e-02_rb,3.186003e-02_rb, &
       2.984290e-02_rb,2.805671e-02_rb,2.645895e-02_rb,2.501733e-02_rb,2.370689e-02_rb, &
       2.250808e-02_rb,2.140532e-02_rb,2.038609e-02_rb,1.944018e-02_rb,1.855918e-02_rb, &
       1.773609e-02_rb,1.696504e-02_rb,1.624106e-02_rb,1.555990e-02_rb,1.491793e-02_rb, &
       1.431197e-02_rb,1.373928e-02_rb,1.319743e-02_rb,1.268430e-02_rb,1.219799e-02_rb, &
       1.173682e-02_rb,1.129925e-02_rb,1.088393e-02_rb,1.048961e-02_rb,1.011516e-02_rb, &
       9.759543e-03_rb,9.421813e-03_rb,9.101089e-03_rb,8.796559e-03_rb,8.507464e-03_rb, &
       8.233098e-03_rb,7.972798e-03_rb,7.725942e-03_rb,7.491940e-03_rb,7.270238e-03_rb, &
       7.060305e-03_rb/)                                                             
      absice3(:,9) = (/ &                                                            
! band 9                                                                             
       1.236780e-01_rb,9.222386e-02_rb,7.383997e-02_rb,6.204072e-02_rb,5.381029e-02_rb, &
       4.770678e-02_rb,4.296928e-02_rb,3.916131e-02_rb,3.601540e-02_rb,3.335878e-02_rb, &
       3.107493e-02_rb,2.908247e-02_rb,2.732282e-02_rb,2.575276e-02_rb,2.433968e-02_rb, &
       2.305852e-02_rb,2.188966e-02_rb,2.081757e-02_rb,1.982974e-02_rb,1.891599e-02_rb, &
       1.806794e-02_rb,1.727865e-02_rb,1.654227e-02_rb,1.585387e-02_rb,1.520924e-02_rb, &
       1.460476e-02_rb,1.403730e-02_rb,1.350416e-02_rb,1.300293e-02_rb,1.253153e-02_rb, &
       1.208808e-02_rb,1.167094e-02_rb,1.127862e-02_rb,1.090979e-02_rb,1.056323e-02_rb, &
       1.023786e-02_rb,9.932665e-03_rb,9.646744e-03_rb,9.379250e-03_rb,9.129409e-03_rb, &
       8.896500e-03_rb,8.679856e-03_rb,8.478852e-03_rb,8.292904e-03_rb,8.121463e-03_rb, &
       7.964013e-03_rb/)                                                             
      absice3(:,10) = (/ &                                                           
! band 10                                                                            
       1.655966e-01_rb,1.134205e-01_rb,8.714344e-02_rb,7.129241e-02_rb,6.063739e-02_rb, &
       5.294203e-02_rb,4.709309e-02_rb,4.247476e-02_rb,3.871892e-02_rb,3.559206e-02_rb, &
       3.293893e-02_rb,3.065226e-02_rb,2.865558e-02_rb,2.689288e-02_rb,2.532221e-02_rb, &
       2.391150e-02_rb,2.263582e-02_rb,2.147549e-02_rb,2.041476e-02_rb,1.944089e-02_rb, &
       1.854342e-02_rb,1.771371e-02_rb,1.694456e-02_rb,1.622989e-02_rb,1.556456e-02_rb, &
       1.494415e-02_rb,1.436491e-02_rb,1.382354e-02_rb,1.331719e-02_rb,1.284339e-02_rb, &
       1.239992e-02_rb,1.198486e-02_rb,1.159647e-02_rb,1.123323e-02_rb,1.089375e-02_rb, &
       1.057679e-02_rb,1.028124e-02_rb,1.000607e-02_rb,9.750376e-03_rb,9.513303e-03_rb, &
       9.294082e-03_rb,9.092003e-03_rb,8.906412e-03_rb,8.736702e-03_rb,8.582314e-03_rb, &
       8.442725e-03_rb/)                                                             
      absice3(:,11) = (/ &                                                           
! band 11                                                                            
       1.775615e-01_rb,1.180046e-01_rb,8.929607e-02_rb,7.233500e-02_rb,6.108333e-02_rb, &
       5.303642e-02_rb,4.696927e-02_rb,4.221206e-02_rb,3.836768e-02_rb,3.518576e-02_rb, &
       3.250063e-02_rb,3.019825e-02_rb,2.819758e-02_rb,2.643943e-02_rb,2.487953e-02_rb, &
       2.348414e-02_rb,2.222705e-02_rb,2.108762e-02_rb,2.004936e-02_rb,1.909892e-02_rb, &
       1.822539e-02_rb,1.741975e-02_rb,1.667449e-02_rb,1.598330e-02_rb,1.534084e-02_rb, &
       1.474253e-02_rb,1.418446e-02_rb,1.366325e-02_rb,1.317597e-02_rb,1.272004e-02_rb, &
       1.229321e-02_rb,1.189350e-02_rb,1.151915e-02_rb,1.116859e-02_rb,1.084042e-02_rb, &
       1.053338e-02_rb,1.024636e-02_rb,9.978326e-03_rb,9.728357e-03_rb,9.495613e-03_rb, &
       9.279327e-03_rb,9.078798e-03_rb,8.893383e-03_rb,8.722488e-03_rb,8.565568e-03_rb, &
       8.422115e-03_rb/)                                                             
      absice3(:,12) = (/ &                                                           
! band 12                                                                            
       9.465447e-02_rb,6.432047e-02_rb,5.060973e-02_rb,4.267283e-02_rb,3.741843e-02_rb, &
       3.363096e-02_rb,3.073531e-02_rb,2.842405e-02_rb,2.651789e-02_rb,2.490518e-02_rb, &
       2.351273e-02_rb,2.229056e-02_rb,2.120335e-02_rb,2.022541e-02_rb,1.933763e-02_rb, &
       1.852546e-02_rb,1.777763e-02_rb,1.708528e-02_rb,1.644134e-02_rb,1.584009e-02_rb, &
       1.527684e-02_rb,1.474774e-02_rb,1.424955e-02_rb,1.377957e-02_rb,1.333549e-02_rb, &
       1.291534e-02_rb,1.251743e-02_rb,1.214029e-02_rb,1.178265e-02_rb,1.144337e-02_rb, &
       1.112148e-02_rb,1.081609e-02_rb,1.052642e-02_rb,1.025178e-02_rb,9.991540e-03_rb, &
       9.745130e-03_rb,9.512038e-03_rb,9.291797e-03_rb,9.083980e-03_rb,8.888195e-03_rb, &
       8.704081e-03_rb,8.531306e-03_rb,8.369560e-03_rb,8.218558e-03_rb,8.078032e-03_rb, &
       7.947730e-03_rb/)                                                             
      absice3(:,13) = (/ &                                                           
! band 13                                                                            
       1.560311e-01_rb,9.961097e-02_rb,7.502949e-02_rb,6.115022e-02_rb,5.214952e-02_rb, &
       4.578149e-02_rb,4.099731e-02_rb,3.724174e-02_rb,3.419343e-02_rb,3.165356e-02_rb, &
       2.949251e-02_rb,2.762222e-02_rb,2.598073e-02_rb,2.452322e-02_rb,2.321642e-02_rb, &
       2.203516e-02_rb,2.096002e-02_rb,1.997579e-02_rb,1.907036e-02_rb,1.823401e-02_rb, &
       1.745879e-02_rb,1.673819e-02_rb,1.606678e-02_rb,1.544003e-02_rb,1.485411e-02_rb, &
       1.430574e-02_rb,1.379215e-02_rb,1.331092e-02_rb,1.285996e-02_rb,1.243746e-02_rb, &
       1.204183e-02_rb,1.167164e-02_rb,1.132567e-02_rb,1.100281e-02_rb,1.070207e-02_rb, &
       1.042258e-02_rb,1.016352e-02_rb,9.924197e-03_rb,9.703953e-03_rb,9.502199e-03_rb, &
       9.318400e-03_rb,9.152066e-03_rb,9.002749e-03_rb,8.870038e-03_rb,8.753555e-03_rb, &
       8.652951e-03_rb/)                                                             
      absice3(:,14) = (/ &                                                           
! band 14                                                                            
       1.559547e-01_rb,9.896700e-02_rb,7.441231e-02_rb,6.061469e-02_rb,5.168730e-02_rb, &
       4.537821e-02_rb,4.064106e-02_rb,3.692367e-02_rb,3.390714e-02_rb,3.139438e-02_rb, &
       2.925702e-02_rb,2.740783e-02_rb,2.578547e-02_rb,2.434552e-02_rb,2.305506e-02_rb, &
       2.188910e-02_rb,2.082842e-02_rb,1.985789e-02_rb,1.896553e-02_rb,1.814165e-02_rb, &
       1.737839e-02_rb,1.666927e-02_rb,1.600891e-02_rb,1.539279e-02_rb,1.481712e-02_rb, &
       1.427865e-02_rb,1.377463e-02_rb,1.330266e-02_rb,1.286068e-02_rb,1.244689e-02_rb, &
       1.205973e-02_rb,1.169780e-02_rb,1.135989e-02_rb,1.104492e-02_rb,1.075192e-02_rb, &
       1.048004e-02_rb,1.022850e-02_rb,9.996611e-03_rb,9.783753e-03_rb,9.589361e-03_rb, &
       9.412924e-03_rb,9.253977e-03_rb,9.112098e-03_rb,8.986903e-03_rb,8.878039e-03_rb, &
       8.785184e-03_rb/)                                                             
      absice3(:,15) = (/ &                                                           
! band 15                                                                            
       1.102926e-01_rb,7.176622e-02_rb,5.530316e-02_rb,4.606056e-02_rb,4.006116e-02_rb, &
       3.579628e-02_rb,3.256909e-02_rb,3.001360e-02_rb,2.791920e-02_rb,2.615617e-02_rb, &
       2.464023e-02_rb,2.331426e-02_rb,2.213817e-02_rb,2.108301e-02_rb,2.012733e-02_rb, &
       1.925493e-02_rb,1.845331e-02_rb,1.771269e-02_rb,1.702531e-02_rb,1.638493e-02_rb, &
       1.578648e-02_rb,1.522579e-02_rb,1.469940e-02_rb,1.420442e-02_rb,1.373841e-02_rb, &
       1.329931e-02_rb,1.288535e-02_rb,1.249502e-02_rb,1.212700e-02_rb,1.178015e-02_rb, &
       1.145348e-02_rb,1.114612e-02_rb,1.085730e-02_rb,1.058633e-02_rb,1.033263e-02_rb, &
       1.009564e-02_rb,9.874895e-03_rb,9.669960e-03_rb,9.480449e-03_rb,9.306014e-03_rb, &
       9.146339e-03_rb,9.001138e-03_rb,8.870154e-03_rb,8.753148e-03_rb,8.649907e-03_rb, &
       8.560232e-03_rb/)                                                             
      absice3(:,16) = (/ &
! band 16                                                                            
       1.688344e-01_rb,1.077072e-01_rb,7.994467e-02_rb,6.403862e-02_rb,5.369850e-02_rb, &
       4.641582e-02_rb,4.099331e-02_rb,3.678724e-02_rb,3.342069e-02_rb,3.065831e-02_rb, &
       2.834557e-02_rb,2.637680e-02_rb,2.467733e-02_rb,2.319286e-02_rb,2.188299e-02_rb, &
       2.071701e-02_rb,1.967121e-02_rb,1.872692e-02_rb,1.786931e-02_rb,1.708641e-02_rb, &
       1.636846e-02_rb,1.570743e-02_rb,1.509665e-02_rb,1.453052e-02_rb,1.400433e-02_rb, &
       1.351407e-02_rb,1.305631e-02_rb,1.262810e-02_rb,1.222688e-02_rb,1.185044e-02_rb, &
       1.149683e-02_rb,1.116436e-02_rb,1.085153e-02_rb,1.055701e-02_rb,1.027961e-02_rb, &
       1.001831e-02_rb,9.772141e-03_rb,9.540280e-03_rb,9.321966e-03_rb,9.116517e-03_rb, &
       8.923315e-03_rb,8.741803e-03_rb,8.571472e-03_rb,8.411860e-03_rb,8.262543e-03_rb, &
       8.123136e-03_rb/)                       
 
! For LIQFLAG = 0.                                                                   
      absliq0 = 0.0903614_rb                                                         
                                                                                     
! For LIQFLAG = 1.  In each band, the absorption                                     
! coefficients are listed for a range of effective radii from 2.5                    
! to 59.5 microns in increments of 1.0 micron.                                       
      absliq1(:, 1) = (/ &                                                           
! band  1                                                                            
       1.64047e-03_rb, 6.90533e-02_rb, 7.72017e-02_rb, 7.78054e-02_rb, 7.69523e-02_rb, &
       7.58058e-02_rb, 7.46400e-02_rb, 7.35123e-02_rb, 7.24162e-02_rb, 7.13225e-02_rb, &
       6.99145e-02_rb, 6.66409e-02_rb, 6.36582e-02_rb, 6.09425e-02_rb, 5.84593e-02_rb, &
       5.61743e-02_rb, 5.40571e-02_rb, 5.20812e-02_rb, 5.02245e-02_rb, 4.84680e-02_rb, &
       4.67959e-02_rb, 4.51944e-02_rb, 4.36516e-02_rb, 4.21570e-02_rb, 4.07015e-02_rb, &
       3.92766e-02_rb, 3.78747e-02_rb, 3.64886e-02_rb, 3.53632e-02_rb, 3.41992e-02_rb, &
       3.31016e-02_rb, 3.20643e-02_rb, 3.10817e-02_rb, 3.01490e-02_rb, 2.92620e-02_rb, &
       2.84171e-02_rb, 2.76108e-02_rb, 2.68404e-02_rb, 2.61031e-02_rb, 2.53966e-02_rb, &
       2.47189e-02_rb, 2.40678e-02_rb, 2.34418e-02_rb, 2.28392e-02_rb, 2.22586e-02_rb, &
       2.16986e-02_rb, 2.11580e-02_rb, 2.06356e-02_rb, 2.01305e-02_rb, 1.96417e-02_rb, &
       1.91682e-02_rb, 1.87094e-02_rb, 1.82643e-02_rb, 1.78324e-02_rb, 1.74129e-02_rb, &
       1.70052e-02_rb, 1.66088e-02_rb, 1.62231e-02_rb/)                              
      absliq1(:, 2) = (/ &                                                           
! band  2                                                                            
       2.19486e-01_rb, 1.80687e-01_rb, 1.59150e-01_rb, 1.44731e-01_rb, 1.33703e-01_rb, &
       1.24355e-01_rb, 1.15756e-01_rb, 1.07318e-01_rb, 9.86119e-02_rb, 8.92739e-02_rb, &
       8.34911e-02_rb, 7.70773e-02_rb, 7.15240e-02_rb, 6.66615e-02_rb, 6.23641e-02_rb, &
       5.85359e-02_rb, 5.51020e-02_rb, 5.20032e-02_rb, 4.91916e-02_rb, 4.66283e-02_rb, &
       4.42813e-02_rb, 4.21236e-02_rb, 4.01330e-02_rb, 3.82905e-02_rb, 3.65797e-02_rb, &
       3.49869e-02_rb, 3.35002e-02_rb, 3.21090e-02_rb, 3.08957e-02_rb, 2.97601e-02_rb, &
       2.86966e-02_rb, 2.76984e-02_rb, 2.67599e-02_rb, 2.58758e-02_rb, 2.50416e-02_rb, &
       2.42532e-02_rb, 2.35070e-02_rb, 2.27997e-02_rb, 2.21284e-02_rb, 2.14904e-02_rb, &
       2.08834e-02_rb, 2.03051e-02_rb, 1.97536e-02_rb, 1.92271e-02_rb, 1.87239e-02_rb, &
       1.82425e-02_rb, 1.77816e-02_rb, 1.73399e-02_rb, 1.69162e-02_rb, 1.65094e-02_rb, &
       1.61187e-02_rb, 1.57430e-02_rb, 1.53815e-02_rb, 1.50334e-02_rb, 1.46981e-02_rb, &
       1.43748e-02_rb, 1.40628e-02_rb, 1.37617e-02_rb/)                              
      absliq1(:, 3) = (/ &                                                           
! band  3                                                                            
       2.95174e-01_rb, 2.34765e-01_rb, 1.98038e-01_rb, 1.72114e-01_rb, 1.52083e-01_rb, &
       1.35654e-01_rb, 1.21613e-01_rb, 1.09252e-01_rb, 9.81263e-02_rb, 8.79448e-02_rb, &
       8.12566e-02_rb, 7.44563e-02_rb, 6.86374e-02_rb, 6.36042e-02_rb, 5.92094e-02_rb, &
       5.53402e-02_rb, 5.19087e-02_rb, 4.88455e-02_rb, 4.60951e-02_rb, 4.36124e-02_rb, &
       4.13607e-02_rb, 3.93096e-02_rb, 3.74338e-02_rb, 3.57119e-02_rb, 3.41261e-02_rb, &
       3.26610e-02_rb, 3.13036e-02_rb, 3.00425e-02_rb, 2.88497e-02_rb, 2.78077e-02_rb, &
       2.68317e-02_rb, 2.59158e-02_rb, 2.50545e-02_rb, 2.42430e-02_rb, 2.34772e-02_rb, &
       2.27533e-02_rb, 2.20679e-02_rb, 2.14181e-02_rb, 2.08011e-02_rb, 2.02145e-02_rb, &
       1.96561e-02_rb, 1.91239e-02_rb, 1.86161e-02_rb, 1.81311e-02_rb, 1.76673e-02_rb, &
       1.72234e-02_rb, 1.67981e-02_rb, 1.63903e-02_rb, 1.59989e-02_rb, 1.56230e-02_rb, &
       1.52615e-02_rb, 1.49138e-02_rb, 1.45791e-02_rb, 1.42565e-02_rb, 1.39455e-02_rb, &
       1.36455e-02_rb, 1.33559e-02_rb, 1.30761e-02_rb/)                              
      absliq1(:, 4) = (/ &                                                           
! band  4                                                                            
       3.00925e-01_rb, 2.36949e-01_rb, 1.96947e-01_rb, 1.68692e-01_rb, 1.47190e-01_rb, &
       1.29986e-01_rb, 1.15719e-01_rb, 1.03568e-01_rb, 9.30028e-02_rb, 8.36658e-02_rb, &
       7.71075e-02_rb, 7.07002e-02_rb, 6.52284e-02_rb, 6.05024e-02_rb, 5.63801e-02_rb, &
       5.27534e-02_rb, 4.95384e-02_rb, 4.66690e-02_rb, 4.40925e-02_rb, 4.17664e-02_rb, &
       3.96559e-02_rb, 3.77326e-02_rb, 3.59727e-02_rb, 3.43561e-02_rb, 3.28662e-02_rb, &
       3.14885e-02_rb, 3.02110e-02_rb, 2.90231e-02_rb, 2.78948e-02_rb, 2.69109e-02_rb, &
       2.59884e-02_rb, 2.51217e-02_rb, 2.43058e-02_rb, 2.35364e-02_rb, 2.28096e-02_rb, &
       2.21218e-02_rb, 2.14700e-02_rb, 2.08515e-02_rb, 2.02636e-02_rb, 1.97041e-02_rb, &
       1.91711e-02_rb, 1.86625e-02_rb, 1.81769e-02_rb, 1.77126e-02_rb, 1.72683e-02_rb, &
       1.68426e-02_rb, 1.64344e-02_rb, 1.60427e-02_rb, 1.56664e-02_rb, 1.53046e-02_rb, &
       1.49565e-02_rb, 1.46214e-02_rb, 1.42985e-02_rb, 1.39871e-02_rb, 1.36866e-02_rb, &
       1.33965e-02_rb, 1.31162e-02_rb, 1.28453e-02_rb/)                              
      absliq1(:, 5) = (/ &                                                           
! band  5                                                                            
       2.64691e-01_rb, 2.12018e-01_rb, 1.78009e-01_rb, 1.53539e-01_rb, 1.34721e-01_rb, &
       1.19580e-01_rb, 1.06996e-01_rb, 9.62772e-02_rb, 8.69710e-02_rb, 7.87670e-02_rb, &
       7.29272e-02_rb, 6.70920e-02_rb, 6.20977e-02_rb, 5.77732e-02_rb, 5.39910e-02_rb, &
       5.06538e-02_rb, 4.76866e-02_rb, 4.50301e-02_rb, 4.26374e-02_rb, 4.04704e-02_rb, &
       3.84981e-02_rb, 3.66948e-02_rb, 3.50394e-02_rb, 3.35141e-02_rb, 3.21038e-02_rb, &
       3.07957e-02_rb, 2.95788e-02_rb, 2.84438e-02_rb, 2.73790e-02_rb, 2.64390e-02_rb, &
       2.55565e-02_rb, 2.47263e-02_rb, 2.39437e-02_rb, 2.32047e-02_rb, 2.25056e-02_rb, &
       2.18433e-02_rb, 2.12149e-02_rb, 2.06177e-02_rb, 2.00495e-02_rb, 1.95081e-02_rb, &
       1.89917e-02_rb, 1.84984e-02_rb, 1.80269e-02_rb, 1.75755e-02_rb, 1.71431e-02_rb, &
       1.67283e-02_rb, 1.63303e-02_rb, 1.59478e-02_rb, 1.55801e-02_rb, 1.52262e-02_rb, &
       1.48853e-02_rb, 1.45568e-02_rb, 1.42400e-02_rb, 1.39342e-02_rb, 1.36388e-02_rb, &
       1.33533e-02_rb, 1.30773e-02_rb, 1.28102e-02_rb/)                              
      absliq1(:, 6) = (/ &                                                           
! band  6                                                                            
       8.81182e-02_rb, 1.06745e-01_rb, 9.79753e-02_rb, 8.99625e-02_rb, 8.35200e-02_rb, &
       7.81899e-02_rb, 7.35939e-02_rb, 6.94696e-02_rb, 6.56266e-02_rb, 6.19148e-02_rb, &
       5.83355e-02_rb, 5.49306e-02_rb, 5.19642e-02_rb, 4.93325e-02_rb, 4.69659e-02_rb, &
       4.48148e-02_rb, 4.28431e-02_rb, 4.10231e-02_rb, 3.93332e-02_rb, 3.77563e-02_rb, &
       3.62785e-02_rb, 3.48882e-02_rb, 3.35758e-02_rb, 3.23333e-02_rb, 3.11536e-02_rb, &
       3.00310e-02_rb, 2.89601e-02_rb, 2.79365e-02_rb, 2.70502e-02_rb, 2.62618e-02_rb, &
       2.55025e-02_rb, 2.47728e-02_rb, 2.40726e-02_rb, 2.34013e-02_rb, 2.27583e-02_rb, &
       2.21422e-02_rb, 2.15522e-02_rb, 2.09869e-02_rb, 2.04453e-02_rb, 1.99260e-02_rb, &
       1.94280e-02_rb, 1.89501e-02_rb, 1.84913e-02_rb, 1.80506e-02_rb, 1.76270e-02_rb, &
       1.72196e-02_rb, 1.68276e-02_rb, 1.64500e-02_rb, 1.60863e-02_rb, 1.57357e-02_rb, &
       1.53975e-02_rb, 1.50710e-02_rb, 1.47558e-02_rb, 1.44511e-02_rb, 1.41566e-02_rb, &
       1.38717e-02_rb, 1.35960e-02_rb, 1.33290e-02_rb/)                              
      absliq1(:, 7) = (/ &                                                           
! band  7                                                                            
       4.32174e-02_rb, 7.36078e-02_rb, 6.98340e-02_rb, 6.65231e-02_rb, 6.41948e-02_rb, &
       6.23551e-02_rb, 6.06638e-02_rb, 5.88680e-02_rb, 5.67124e-02_rb, 5.38629e-02_rb, &
       4.99579e-02_rb, 4.86289e-02_rb, 4.70120e-02_rb, 4.52854e-02_rb, 4.35466e-02_rb, &
       4.18480e-02_rb, 4.02169e-02_rb, 3.86658e-02_rb, 3.71992e-02_rb, 3.58168e-02_rb, &
       3.45155e-02_rb, 3.32912e-02_rb, 3.21390e-02_rb, 3.10538e-02_rb, 3.00307e-02_rb, &
       2.90651e-02_rb, 2.81524e-02_rb, 2.72885e-02_rb, 2.62821e-02_rb, 2.55744e-02_rb, &
       2.48799e-02_rb, 2.42029e-02_rb, 2.35460e-02_rb, 2.29108e-02_rb, 2.22981e-02_rb, &
       2.17079e-02_rb, 2.11402e-02_rb, 2.05945e-02_rb, 2.00701e-02_rb, 1.95663e-02_rb, &
       1.90824e-02_rb, 1.86174e-02_rb, 1.81706e-02_rb, 1.77411e-02_rb, 1.73281e-02_rb, &
       1.69307e-02_rb, 1.65483e-02_rb, 1.61801e-02_rb, 1.58254e-02_rb, 1.54835e-02_rb, &
       1.51538e-02_rb, 1.48358e-02_rb, 1.45288e-02_rb, 1.42322e-02_rb, 1.39457e-02_rb, &
       1.36687e-02_rb, 1.34008e-02_rb, 1.31416e-02_rb/)                              
      absliq1(:, 8) = (/ &                                                           
! band  8                                                                            
       1.41881e-01_rb, 7.15419e-02_rb, 6.30335e-02_rb, 6.11132e-02_rb, 6.01931e-02_rb, &
       5.92420e-02_rb, 5.78968e-02_rb, 5.58876e-02_rb, 5.28923e-02_rb, 4.84462e-02_rb, &
       4.60839e-02_rb, 4.56013e-02_rb, 4.45410e-02_rb, 4.31866e-02_rb, 4.17026e-02_rb, &
       4.01850e-02_rb, 3.86892e-02_rb, 3.72461e-02_rb, 3.58722e-02_rb, 3.45749e-02_rb, &
       3.33564e-02_rb, 3.22155e-02_rb, 3.11494e-02_rb, 3.01541e-02_rb, 2.92253e-02_rb, &
       2.83584e-02_rb, 2.75488e-02_rb, 2.67925e-02_rb, 2.57692e-02_rb, 2.50704e-02_rb, &
       2.43918e-02_rb, 2.37350e-02_rb, 2.31005e-02_rb, 2.24888e-02_rb, 2.18996e-02_rb, &
       2.13325e-02_rb, 2.07870e-02_rb, 2.02623e-02_rb, 1.97577e-02_rb, 1.92724e-02_rb, &
       1.88056e-02_rb, 1.83564e-02_rb, 1.79241e-02_rb, 1.75079e-02_rb, 1.71070e-02_rb, &
       1.67207e-02_rb, 1.63482e-02_rb, 1.59890e-02_rb, 1.56424e-02_rb, 1.53077e-02_rb, &
       1.49845e-02_rb, 1.46722e-02_rb, 1.43702e-02_rb, 1.40782e-02_rb, 1.37955e-02_rb, &
       1.35219e-02_rb, 1.32569e-02_rb, 1.30000e-02_rb/)                              
      absliq1(:, 9) = (/ &                                                           
! band  9                                                                            
       6.72726e-02_rb, 6.61013e-02_rb, 6.47866e-02_rb, 6.33780e-02_rb, 6.18985e-02_rb, &
       6.03335e-02_rb, 5.86136e-02_rb, 5.65876e-02_rb, 5.39839e-02_rb, 5.03536e-02_rb, &
       4.71608e-02_rb, 4.63630e-02_rb, 4.50313e-02_rb, 4.34526e-02_rb, 4.17876e-02_rb, &
       4.01261e-02_rb, 3.85171e-02_rb, 3.69860e-02_rb, 3.55442e-02_rb, 3.41954e-02_rb, &
       3.29384e-02_rb, 3.17693e-02_rb, 3.06832e-02_rb, 2.96745e-02_rb, 2.87374e-02_rb, &
       2.78662e-02_rb, 2.70557e-02_rb, 2.63008e-02_rb, 2.52450e-02_rb, 2.45424e-02_rb, &
       2.38656e-02_rb, 2.32144e-02_rb, 2.25885e-02_rb, 2.19873e-02_rb, 2.14099e-02_rb, &
       2.08554e-02_rb, 2.03230e-02_rb, 1.98116e-02_rb, 1.93203e-02_rb, 1.88482e-02_rb, &
       1.83944e-02_rb, 1.79578e-02_rb, 1.75378e-02_rb, 1.71335e-02_rb, 1.67440e-02_rb, &
       1.63687e-02_rb, 1.60069e-02_rb, 1.56579e-02_rb, 1.53210e-02_rb, 1.49958e-02_rb, &
       1.46815e-02_rb, 1.43778e-02_rb, 1.40841e-02_rb, 1.37999e-02_rb, 1.35249e-02_rb, &
       1.32585e-02_rb, 1.30004e-02_rb, 1.27502e-02_rb/)                              
      absliq1(:,10) = (/ &                                                           
! band 10                                                                            
       7.97040e-02_rb, 7.63844e-02_rb, 7.36499e-02_rb, 7.13525e-02_rb, 6.93043e-02_rb, &
       6.72807e-02_rb, 6.50227e-02_rb, 6.22395e-02_rb, 5.86093e-02_rb, 5.37815e-02_rb, &
       5.14682e-02_rb, 4.97214e-02_rb, 4.77392e-02_rb, 4.56961e-02_rb, 4.36858e-02_rb, &
       4.17569e-02_rb, 3.99328e-02_rb, 3.82224e-02_rb, 3.66265e-02_rb, 3.51416e-02_rb, &
       3.37617e-02_rb, 3.24798e-02_rb, 3.12887e-02_rb, 3.01812e-02_rb, 2.91505e-02_rb, &
       2.81900e-02_rb, 2.72939e-02_rb, 2.64568e-02_rb, 2.54165e-02_rb, 2.46832e-02_rb, &
       2.39783e-02_rb, 2.33017e-02_rb, 2.26531e-02_rb, 2.20314e-02_rb, 2.14359e-02_rb, &
       2.08653e-02_rb, 2.03187e-02_rb, 1.97947e-02_rb, 1.92924e-02_rb, 1.88106e-02_rb, &
       1.83483e-02_rb, 1.79043e-02_rb, 1.74778e-02_rb, 1.70678e-02_rb, 1.66735e-02_rb, &
       1.62941e-02_rb, 1.59286e-02_rb, 1.55766e-02_rb, 1.52371e-02_rb, 1.49097e-02_rb, &
       1.45937e-02_rb, 1.42885e-02_rb, 1.39936e-02_rb, 1.37085e-02_rb, 1.34327e-02_rb, &
       1.31659e-02_rb, 1.29075e-02_rb, 1.26571e-02_rb/)                              
      absliq1(:,11) = (/ &                                                           
! band 11                                                                            
       1.49438e-01_rb, 1.33535e-01_rb, 1.21542e-01_rb, 1.11743e-01_rb, 1.03263e-01_rb, &
       9.55774e-02_rb, 8.83382e-02_rb, 8.12943e-02_rb, 7.42533e-02_rb, 6.70609e-02_rb, &
       6.38761e-02_rb, 5.97788e-02_rb, 5.59841e-02_rb, 5.25318e-02_rb, 4.94132e-02_rb, &
       4.66014e-02_rb, 4.40644e-02_rb, 4.17706e-02_rb, 3.96910e-02_rb, 3.77998e-02_rb, &
       3.60742e-02_rb, 3.44947e-02_rb, 3.30442e-02_rb, 3.17079e-02_rb, 3.04730e-02_rb, &
       2.93283e-02_rb, 2.82642e-02_rb, 2.72720e-02_rb, 2.61789e-02_rb, 2.53277e-02_rb, &
       2.45237e-02_rb, 2.37635e-02_rb, 2.30438e-02_rb, 2.23615e-02_rb, 2.17140e-02_rb, &
       2.10987e-02_rb, 2.05133e-02_rb, 1.99557e-02_rb, 1.94241e-02_rb, 1.89166e-02_rb, &
       1.84317e-02_rb, 1.79679e-02_rb, 1.75238e-02_rb, 1.70983e-02_rb, 1.66901e-02_rb, &
       1.62983e-02_rb, 1.59219e-02_rb, 1.55599e-02_rb, 1.52115e-02_rb, 1.48761e-02_rb, &
       1.45528e-02_rb, 1.42411e-02_rb, 1.39402e-02_rb, 1.36497e-02_rb, 1.33690e-02_rb, &
       1.30976e-02_rb, 1.28351e-02_rb, 1.25810e-02_rb/)                              
      absliq1(:,12) = (/ &                                                           
! band 12                                                                            
       3.71985e-02_rb, 3.88586e-02_rb, 3.99070e-02_rb, 4.04351e-02_rb, 4.04610e-02_rb, &
       3.99834e-02_rb, 3.89953e-02_rb, 3.74886e-02_rb, 3.54551e-02_rb, 3.28870e-02_rb, &
       3.32576e-02_rb, 3.22444e-02_rb, 3.12384e-02_rb, 3.02584e-02_rb, 2.93146e-02_rb, &
       2.84120e-02_rb, 2.75525e-02_rb, 2.67361e-02_rb, 2.59618e-02_rb, 2.52280e-02_rb, &
       2.45327e-02_rb, 2.38736e-02_rb, 2.32487e-02_rb, 2.26558e-02_rb, 2.20929e-02_rb, &
       2.15579e-02_rb, 2.10491e-02_rb, 2.05648e-02_rb, 1.99749e-02_rb, 1.95704e-02_rb, &
       1.91731e-02_rb, 1.87839e-02_rb, 1.84032e-02_rb, 1.80315e-02_rb, 1.76689e-02_rb, &
       1.73155e-02_rb, 1.69712e-02_rb, 1.66362e-02_rb, 1.63101e-02_rb, 1.59928e-02_rb, &
       1.56842e-02_rb, 1.53840e-02_rb, 1.50920e-02_rb, 1.48080e-02_rb, 1.45318e-02_rb, &
       1.42631e-02_rb, 1.40016e-02_rb, 1.37472e-02_rb, 1.34996e-02_rb, 1.32586e-02_rb, &
       1.30239e-02_rb, 1.27954e-02_rb, 1.25728e-02_rb, 1.23559e-02_rb, 1.21445e-02_rb, &
       1.19385e-02_rb, 1.17376e-02_rb, 1.15417e-02_rb/)                              
 
      absliq1(:,13) = (/ &                                                           
! band 13                                                                            
       3.11868e-02_rb, 4.48357e-02_rb, 4.90224e-02_rb, 4.96406e-02_rb, 4.86806e-02_rb, &
       4.69610e-02_rb, 4.48630e-02_rb, 4.25795e-02_rb, 4.02138e-02_rb, 3.78236e-02_rb, &
       3.74266e-02_rb, 3.60384e-02_rb, 3.47074e-02_rb, 3.34434e-02_rb, 3.22499e-02_rb, &
       3.11264e-02_rb, 3.00704e-02_rb, 2.90784e-02_rb, 2.81463e-02_rb, 2.72702e-02_rb, &
       2.64460e-02_rb, 2.56698e-02_rb, 2.49381e-02_rb, 2.42475e-02_rb, 2.35948e-02_rb, &
       2.29774e-02_rb, 2.23925e-02_rb, 2.18379e-02_rb, 2.11793e-02_rb, 2.07076e-02_rb, &
       2.02470e-02_rb, 1.97981e-02_rb, 1.93613e-02_rb, 1.89367e-02_rb, 1.85243e-02_rb, &
       1.81240e-02_rb, 1.77356e-02_rb, 1.73588e-02_rb, 1.69935e-02_rb, 1.66392e-02_rb, &
       1.62956e-02_rb, 1.59624e-02_rb, 1.56393e-02_rb, 1.53259e-02_rb, 1.50219e-02_rb, &
       1.47268e-02_rb, 1.44404e-02_rb, 1.41624e-02_rb, 1.38925e-02_rb, 1.36302e-02_rb, &
       1.33755e-02_rb, 1.31278e-02_rb, 1.28871e-02_rb, 1.26530e-02_rb, 1.24253e-02_rb, &
       1.22038e-02_rb, 1.19881e-02_rb, 1.17782e-02_rb/)                              
      absliq1(:,14) = (/ &                                                           
! band 14                                                                            
       1.58988e-02_rb, 3.50652e-02_rb, 4.00851e-02_rb, 4.07270e-02_rb, 3.98101e-02_rb, &
       3.83306e-02_rb, 3.66829e-02_rb, 3.50327e-02_rb, 3.34497e-02_rb, 3.19609e-02_rb, &
       3.13712e-02_rb, 3.03348e-02_rb, 2.93415e-02_rb, 2.83973e-02_rb, 2.75037e-02_rb, &
       2.66604e-02_rb, 2.58654e-02_rb, 2.51161e-02_rb, 2.44100e-02_rb, 2.37440e-02_rb, &
       2.31154e-02_rb, 2.25215e-02_rb, 2.19599e-02_rb, 2.14282e-02_rb, 2.09242e-02_rb, &
       2.04459e-02_rb, 1.99915e-02_rb, 1.95594e-02_rb, 1.90254e-02_rb, 1.86598e-02_rb, &
       1.82996e-02_rb, 1.79455e-02_rb, 1.75983e-02_rb, 1.72584e-02_rb, 1.69260e-02_rb, &
       1.66013e-02_rb, 1.62843e-02_rb, 1.59752e-02_rb, 1.56737e-02_rb, 1.53799e-02_rb, &
       1.50936e-02_rb, 1.48146e-02_rb, 1.45429e-02_rb, 1.42782e-02_rb, 1.40203e-02_rb, &
       1.37691e-02_rb, 1.35243e-02_rb, 1.32858e-02_rb, 1.30534e-02_rb, 1.28270e-02_rb, &
       1.26062e-02_rb, 1.23909e-02_rb, 1.21810e-02_rb, 1.19763e-02_rb, 1.17766e-02_rb, &
       1.15817e-02_rb, 1.13915e-02_rb, 1.12058e-02_rb/)                              
      absliq1(:,15) = (/ &                                                           
! band 15                                                                            
       5.02079e-03_rb, 2.17615e-02_rb, 2.55449e-02_rb, 2.59484e-02_rb, 2.53650e-02_rb, &
       2.45281e-02_rb, 2.36843e-02_rb, 2.29159e-02_rb, 2.22451e-02_rb, 2.16716e-02_rb, &
       2.11451e-02_rb, 2.05817e-02_rb, 2.00454e-02_rb, 1.95372e-02_rb, 1.90567e-02_rb, &
       1.86028e-02_rb, 1.81742e-02_rb, 1.77693e-02_rb, 1.73866e-02_rb, 1.70244e-02_rb, &
       1.66815e-02_rb, 1.63563e-02_rb, 1.60477e-02_rb, 1.57544e-02_rb, 1.54755e-02_rb, &
       1.52097e-02_rb, 1.49564e-02_rb, 1.47146e-02_rb, 1.43684e-02_rb, 1.41728e-02_rb, &
       1.39762e-02_rb, 1.37797e-02_rb, 1.35838e-02_rb, 1.33891e-02_rb, 1.31961e-02_rb, &
       1.30051e-02_rb, 1.28164e-02_rb, 1.26302e-02_rb, 1.24466e-02_rb, 1.22659e-02_rb, &
       1.20881e-02_rb, 1.19131e-02_rb, 1.17412e-02_rb, 1.15723e-02_rb, 1.14063e-02_rb, &
       1.12434e-02_rb, 1.10834e-02_rb, 1.09264e-02_rb, 1.07722e-02_rb, 1.06210e-02_rb, &
       1.04725e-02_rb, 1.03269e-02_rb, 1.01839e-02_rb, 1.00436e-02_rb, 9.90593e-03_rb, &
       9.77080e-03_rb, 9.63818e-03_rb, 9.50800e-03_rb/)                              
      absliq1(:,16) = (/ &                                                           
! band 16                                                                            
       5.64971e-02_rb, 9.04736e-02_rb, 8.11726e-02_rb, 7.05450e-02_rb, 6.20052e-02_rb, &
       5.54286e-02_rb, 5.03503e-02_rb, 4.63791e-02_rb, 4.32290e-02_rb, 4.06959e-02_rb, &
       3.74690e-02_rb, 3.52964e-02_rb, 3.33799e-02_rb, 3.16774e-02_rb, 3.01550e-02_rb, &
       2.87856e-02_rb, 2.75474e-02_rb, 2.64223e-02_rb, 2.53953e-02_rb, 2.44542e-02_rb, &
       2.35885e-02_rb, 2.27894e-02_rb, 2.20494e-02_rb, 2.13622e-02_rb, 2.07222e-02_rb, &
       2.01246e-02_rb, 1.95654e-02_rb, 1.90408e-02_rb, 1.84398e-02_rb, 1.80021e-02_rb, &
       1.75816e-02_rb, 1.71775e-02_rb, 1.67889e-02_rb, 1.64152e-02_rb, 1.60554e-02_rb, &
       1.57089e-02_rb, 1.53751e-02_rb, 1.50531e-02_rb, 1.47426e-02_rb, 1.44428e-02_rb, &
       1.41532e-02_rb, 1.38734e-02_rb, 1.36028e-02_rb, 1.33410e-02_rb, 1.30875e-02_rb, &
       1.28420e-02_rb, 1.26041e-02_rb, 1.23735e-02_rb, 1.21497e-02_rb, 1.19325e-02_rb, &
       1.17216e-02_rb, 1.15168e-02_rb, 1.13177e-02_rb, 1.11241e-02_rb, 1.09358e-02_rb, &
       1.07525e-02_rb, 1.05741e-02_rb, 1.04003e-02_rb/)                              
 
!jm not thread safe      hvrclc = '$Revision: 1.8 $'
 
      ncbands = 1
 
! This initialization is done in rrtmg_lw_subcol.F90.
!      do lay = 1, nlayers
!         do ig = 1, ngptlw
!            taucmc(ig,lay) = 0.0_rb
!         enddo
!      enddo
 
! Main layer loop
      do lay = 1, nlayers
 
        do ig = 1, ngptlw
          cwp = ciwpmc(ig,lay) + clwpmc(ig,lay) + cswpmc(ig,lay)
          if (cldfmc(ig,lay) .ge. cldmin .and.                          &
     &      (cwp .ge. cldmin .or. taucmc(ig,lay) .ge. cldmin)) then
 
 
! Ice clouds and water clouds combined.
            if (inflag .eq. 0) then
! Cloud optical depth already defined in taucmc, return to main program
               return
 
            elseif(inflag .eq. 1) then
                errflg = 1
                errmsg = 'ERROR(rlwinit): INFLAG = 1 OPTION NOT AVAILABLE WITH MCICA'
                return
!               cwp = ciwpmc(ig,lay) + clwpmc(ig,lay)
!               taucmc(ig,lay) = abscld1 * cwp
 
! Separate treatement of ice clouds and water clouds.
            elseif(inflag .ge. 2) then
               radice = reicmc(lay)
 
! Calculation of absorption coefficients due to ice clouds.
               if ((ciwpmc(ig,lay)+cswpmc(ig,lay)) .eq. 0.0_rb) then
                  abscoice(ig) = 0.0_rb
                  abscosno(ig) = 0.0_rb
 
               elseif (iceflag .eq. 0) then
!                  if (radice .lt. 10.0_rb) stop 'ICE RADIUS TOO SMALL'
                  abscoice(ig) = absice0(1) + absice0(2)/max(radice,10.0_rb)
                  abscosno(ig) = 0.0_rb
 
               elseif (iceflag .eq. 1) then
!                  if (radice .lt. 13.0_rb .or. radice .gt. 130._rb) stop&
!     &                'ICE RADIUS OUT OF BOUNDS'
                  ncbands = 5
                  ib = icb(ngb(ig))
                  abscoice(ig) = absice1(1,ib) + absice1(2,ib)/min(max(radice,13.0_rb),130._rb)
                  abscosno(ig) = 0.0_rb
 
! For iceflag=2 option, ice particle effective radius is limited to 5.0 to 131.0 microns
 
               elseif (iceflag .eq. 2) then
!                  if (radice .lt. 5.0_rb .or. radice .gt. 131.0_rb) stop&
!     &                'ICE RADIUS OUT OF BOUNDS'
                     ncbands = 16
                     factor = (min(max(radice,5.0_rb),131._rb) - 2._rb)/3._rb
                     index = int(factor)
                     if (index .eq. 43) index = 42
                     fint = factor - float(index)
                     ib = ngb(ig)
                     abscoice(ig) =                                     &
     &                   absice2(index,ib) + fint *                     &
     &                   (absice2(index+1,ib) - (absice2(index,ib)))
                     abscosno(ig) = 0.0_rb
 
! For iceflag=3 option, ice particle generalized effective size is limited to 5.0 to 140.0 microns
 
               elseif (iceflag .ge. 3) then
!                  if (radice .lt. 5.0_rb .or. radice .gt. 140.0_rb) then
!                         write(errmsg,'(a,i5,i5,f8.2,f8.2)' )           &
!     &         'ERROR: ICE GENERALIZED EFFECTIVE SIZE OUT OF BOUNDS'    &
!     &          ,ig, lay, ciwpmc(ig,lay), radice
!                         errflg = 1
!                         return
!                     end if                                                                      
                     ncbands = 16                                                                
                     factor = (min(max(radice,5.0_rb),140._rb) - 2._rb)/3._rb                    
                     index = int(factor)                                                         
                     if (index .eq. 46) index = 45                                               
                     fint = factor - float(index)                                                
                     ib = ngb(ig)                                                                
                     abscoice(ig) =                                     &
     &                   absice3(index,ib) + fint *                     &
     &                   (absice3(index+1,ib) - (absice3(index,ib)))                             
                     abscosno(ig) = 0.0_rb                                                       
                                                                                                 
               endif                                                                             
                                                                                                 
!..Incorporate additional effects due to snow.                                                   
               if (cswpmc(ig,lay).gt.0.0_rb .and. iceflag .eq. 5) then                           
                  radsno = resnmc(lay)                                                           
!                  if (radsno .lt. 5.0_rb .or. radsno .gt. 140.0_rb) then                         
!                         write(errmsg,'(a,i5,i5,f8.2,f8.2)' )           &
!     &         'ERROR: SNOW GENERALIZED EFFECTIVE SIZE OUT OF BOUNDS'   &                        
!     &         ,ig, lay, cswpmc(ig,lay), radsno                                                  
!                         errflg = 1
!                         return
!                     end if                                                                      
                     ncbands = 16                                                                
                     factor = (min(max(radsno,5.0_rb),140.0_rb) - 2._rb)/3._rb                   
                     index = int(factor)                                                         
                     if (index .eq. 46) index = 45                                               
                     fint = factor - float(index)                                                
                     ib = ngb(ig)                                                                
                     abscosno(ig) =                                     &
     &                   absice3(index,ib) + fint *                     &
     &                  (absice3(index+1,ib) - (absice3(index,ib)))                             
               endif                                                                             
                                                                                                 
                                                                                                 
                                                                                                 
! Calculation of absorption coefficients due to water clouds.                                    
               if (clwpmc(ig,lay) .eq. 0.0_rb) then                                              
                  abscoliq(ig) = 0.0_rb                                                          
                                                                                                 
               elseif (liqflag .eq. 0) then                                                      
                   abscoliq(ig) = absliq0                                                        
                                                                                                 
               elseif (liqflag .eq. 1) then                                                      
                  radliq = relqmc(lay)                        
!                  if (radliq .lt. 2.5_rb .or. radliq .gt. 60._rb) then
!                     write(errmsg,'(a,i5,i5,f8.2,f8.2)' )              &
!&                         'ERROR: LIQUID EFFECTIVE SIZE OUT OF BOUNDS' &
!&                         ,ig, lay, clwpmc(ig,lay), radliq
!                     errflg = 1
!                     return
!                  end if
                  index = int(min(max(radliq,2.5_rb),60._rb) - 1.5_rb)                           
                  if (index .eq. 0) index = 1                                                    
                  if (index .eq. 58) index = 57                                                  
                  fint = radliq - 1.5_rb - float(index)                                          
                  ib = ngb(ig)                                                                   
                  abscoliq(ig) =                                        &
     &                  absliq1(index,ib) + fint *                      &
     &                  (absliq1(index+1,ib) - (absliq1(index,ib)))                              
               endif                                                                             
                                                                                                 
               taucmc(ig,lay) = ciwpmc(ig,lay) * abscoice(ig) +         &
     &                           clwpmc(ig,lay) * abscoliq(ig) +        &
     &                           cswpmc(ig,lay) * abscosno(ig)                                    
                                                                                                 
            endif                                                                                
         endif                                                                                   
         enddo                                                                                   
      enddo                                                                                      
                                                                                                 
      end subroutine cldprmc                                                                     
                                                                    
!........................................!$
      end module rrtmg_lw                !$
!========================================!$