Common Community Physics Package (CCPP) Scientific Documentation  Version 2.0
rrtmg_lw Module Reference

This module contains the CCPP-compliant NCEP's modifications of the rrtm-lw radiation code from aer inc.

Functions/Subroutines

subroutine, public rrtmg_lw_init ()
 
subroutine, public rrtmg_lw_run (plyr, plvl, tlyr, tlvl, qlyr, olyr, gasvmr_co2, gasvmr_n2o, gasvmr_ch4, gasvmr_o2, gasvmr_co, gasvmr_cfc11, gasvmr_cfc12, gasvmr_cfc22, gasvmr_ccl4, icseed, aeraod, aerssa, sfemis, sfgtmp, npts, nlay, nlp1, lprnt, cld_cf, lslwr, hlwc, topflx, sfcflx, HLW0, HLWB, FLXPRF, cld_lwp, cld_ref_liq, cld_iwp, cld_ref_ice, cld_rwp, cld_ref_rain, cld_swp, cld_ref_snow, cld_od_total, cld_od_layer, cld_od, errmsg, errflg )
 
subroutine, public rrtmg_lw_finalize ()
 
subroutine, public rlwinit (me)
 This subroutine performs calculations necessary for the initialization of the longwave model, which includes non-varying model variables, conversion factors, and look-up tables. More...
 
subroutine cldprop (cfrac, cliqp, reliq, cicep, reice, cdat1, cdat2, cdat3, cdat4, nlay, nlp1, ipseed, cldfmc, taucld )
 This subroutine computes the cloud optical depth(s) for each cloudy layer and g-point interval. More...
 
subroutine mcica_subcol (cldf, nlay, ipseed, lcloudy )
 This suroutine computes sub-colum cloud profile flag array. More...
 
subroutine setcoef (pavel, tavel, tz, stemp, h2ovmr, colamt, coldry, colbrd, nlay, nlp1, laytrop, pklay, pklev, jp, jt, jt1, rfrate, fac00, fac01, fac10, fac11, selffac, selffrac, indself, forfac, forfrac, indfor, minorfrac, scaleminor, scaleminorn2, indminor )
 This subroutine computes various coefficients needed in radiative transfer calculations. More...
 
subroutine rtrn (semiss, delp, cldfrc, taucld, tautot, pklay, pklev, fracs, secdif, nlay, nlp1, totuflux, totdflux, htr, totuclfl, totdclfl, htrcl, htrb )
 This subroutine computes the upward/downward radiative fluxes, and heating rates for both clear or cloudy atmosphere. Clouds assumed as randomly overlaping in a vertical column. More...
 
subroutine rtrnmr (semiss, delp, cldfrc, taucld, tautot, pklay, pklev, fracs, secdif, nlay, nlp1, totuflux, totdflux, htr, totuclfl, totdclfl, htrcl, htrb )
 This subroutine computes 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 column. More...
 
subroutine rtrnmc (semiss, delp, cldfmc, taucld, tautot, pklay, pklev, fracs, secdif, nlay, nlp1, totuflux, totdflux, htr, totuclfl, totdclfl, htrcl, htrb )
 This subroutine computes the upward/downward radiative fluxes, and heating rates for both clear or cloudy atmosphere.Clouds are treated with the mcica stochastic approach. More...
 
subroutine taumol (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, fracs, tautot )
 This subroutine contains optical depths developed for the rapid radiative transfer model. More...
 

Variables

character(40), parameter vtaglw ='NCEP LW v5.1 Nov 2012 -RRTMG-LW v4.82 '
 
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
 
real(kind=kind_phys), parameter stpfac = 296.0/1013.0
 
real(kind=kind_phys), parameter wtdiff = 0.5
 
real(kind=kind_phys), parameter tblint = ntbl
 
real(kind=kind_phys), parameter f_zero = 0.0
 
real(kind=kind_phys), parameter f_one = 1.0
 
real(kind=kind_phys), parameter amdw = con_amd/con_amw
 
real(kind=kind_phys), parameter amdo3 = con_amd/con_amo3
 
integer, dimension(nbands) nspa
 
integer, dimension(nbands) nspb
 
real(kind=kind_phys), dimension(nbands) a0
 
real(kind=kind_phys), dimension(nbands) a1
 
real(kind=kind_phys), dimension(nbands) a2
 
logical lhlwb = .false.
 
logical lhlw0 = .false.
 
logical lflxprf = .false.
 
real(kind=kind_phys) fluxfac
 
real(kind=kind_phys) heatfac
 
real(kind=kind_phys), dimension(nbands) semiss0
 
real(kind=kind_phys), dimension(0:ntbl) tau_tbl
 clr-sky opt dep (for cldy transfer) More...
 
real(kind=kind_phys), dimension(0:ntbl) exp_tbl
 transmittance lookup table More...
 
real(kind=kind_phys), dimension(0:ntbl) tfn_tbl
 tau transition function; i.e. the transition of planck func from mean lyr temp to lyr boundary temp as a func of opt dep. "linear in tau" method is used. More...
 
integer, parameter ipsdlw0 = ngptlw