GCC Code Coverage Report
Directory: ./ Exec Total Coverage
File: phylmd/rrtm/rrtm_ecrt_140gp.F90 Lines: 103 118 87.3 %
Date: 2023-06-30 12:56:34 Branches: 41 58 70.7 %

Line Branch Exec Source
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!
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! $Id: rrtm_ecrt_140gp.F90 2626 2016-09-15 14:20:56Z musat $
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!
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!****************** SUBROUTINE RRTM_ECRT_140GP **************************
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SUBROUTINE RRTM_ECRT_140GP &
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 & ( K_IPLON, klon , klev, kcld,&
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 & paer , paph , pap,&
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 & pts  , pth  , pt,&
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 & P_ZEMIS, P_ZEMIW,&
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 & pq   , pcco2, pozn, pcldf, ptaucld, ptclear,&
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 & P_CLDFRAC,P_TAUCLD,&
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 & PTAU_LW,&
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 & P_COLDRY,P_WKL,P_WX,&
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 & P_TAUAERL,PAVEL,P_TAVEL,PZ,P_TZ,P_TBOUND,K_NLAYERS,P_SEMISS,K_IREFLECT )
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!     Reformatted for F90 by JJMorcrette, ECMWF, 980714
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!     Read in atmospheric profile from ECMWF radiation code, and prepare it
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!     for use in RRTM.  Set other RRTM input parameters.  Values are passed
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!     back through existing RRTM arrays and commons.
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!- Modifications
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!     2000-05-15 Deborah Salmond  Speed-up
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USE PARKIND1  ,ONLY : JPIM     ,JPRB
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USE YOMHOOK   ,ONLY : LHOOK,   DR_HOOK
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USE PARRRTM  , ONLY : JPBAND   ,JPXSEC   ,JPLAY   ,&
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 & JPINPX
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USE YOERAD   , ONLY : NLW      ,NOVLP
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!MPL/IM 20160915 on prend GES de phylmd USE YOERDI   , ONLY :    RCH4     ,RN2O    ,RCFC11  ,RCFC12
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USE YOESW    , ONLY : RAER
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!------------------------------Arguments--------------------------------
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IMPLICIT NONE
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INTEGER(KIND=JPIM),INTENT(IN)    :: KLON! Number of atmospheres (longitudes)
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INTEGER(KIND=JPIM),INTENT(IN)    :: KLEV! Number of atmospheric layers
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INTEGER(KIND=JPIM),INTENT(IN)    :: K_IPLON
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INTEGER(KIND=JPIM),INTENT(OUT)   :: KCLD
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PAER(KLON,6,KLEV) ! Aerosol optical thickness
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PAPH(KLON,KLEV+1) ! Interface pressures (Pa)
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PAP(KLON,KLEV) ! Layer pressures (Pa)
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PTS(KLON) ! Surface temperature (K)
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PTH(KLON,KLEV+1) ! Interface temperatures (K)
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PT(KLON,KLEV) ! Layer temperature (K)
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REAL(KIND=JPRB)   ,INTENT(IN)    :: P_ZEMIS(KLON) ! Non-window surface emissivity
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REAL(KIND=JPRB)   ,INTENT(IN)    :: P_ZEMIW(KLON) ! Window surface emissivity
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PQ(KLON,KLEV) ! H2O specific humidity (mmr)
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PCCO2 ! CO2 mass mixing ratio
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REAL(KIND=JPRB)   ,INTENT(IN)    :: POZN(KLON,KLEV) ! O3 mass mixing ratio
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PCLDF(KLON,KLEV) ! Cloud fraction
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PTAUCLD(KLON,KLEV,JPBAND) ! Cloud optical depth
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!--C.Kleinschmitt
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REAL(KIND=JPRB)   ,INTENT(IN)    :: PTAU_LW(KLON,KLEV,NLW) ! LW Optical depth of aerosols
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!--end
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: PTCLEAR
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_CLDFRAC(JPLAY) ! Cloud fraction
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_TAUCLD(JPLAY,JPBAND) ! Spectral optical thickness
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_COLDRY(JPLAY)
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_WKL(JPINPX,JPLAY)
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_WX(JPXSEC,JPLAY) ! Amount of trace gases
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_TAUAERL(JPLAY,JPBAND)
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: PAVEL(JPLAY)
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_TAVEL(JPLAY)
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: PZ(0:JPLAY)
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_TZ(0:JPLAY)
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_TBOUND
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INTEGER(KIND=JPIM),INTENT(OUT)   :: K_NLAYERS
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REAL(KIND=JPRB)   ,INTENT(OUT)   :: P_SEMISS(JPBAND)
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INTEGER(KIND=JPIM),INTENT(OUT)   :: K_IREFLECT
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!      real rch4                       ! CH4 mass mixing ratio
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!      real rn2o                       ! N2O mass mixing ratio
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!      real rcfc11                     ! CFC11 mass mixing ratio
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!      real rcfc12                     ! CFC12 mass mixing ratio
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!- from AER
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!- from PROFILE
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!- from SURFACE
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REAL(KIND=JPRB) :: ztauaer(5)
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REAL(KIND=JPRB) :: zc1j(0:klev)               ! total cloud from top and level k
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REAL(KIND=JPRB) :: Z_AMD                  ! Effective molecular weight of dry air (g/mol)
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REAL(KIND=JPRB) :: Z_AMW                  ! Molecular weight of water vapor (g/mol)
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REAL(KIND=JPRB) :: Z_AMCO2                ! Molecular weight of carbon dioxide (g/mol)
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REAL(KIND=JPRB) :: Z_AMO                  ! Molecular weight of ozone (g/mol)
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REAL(KIND=JPRB) :: Z_AMCH4                ! Molecular weight of methane (g/mol)
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REAL(KIND=JPRB) :: Z_AMN2O                ! Molecular weight of nitrous oxide (g/mol)
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REAL(KIND=JPRB) :: Z_AMC11                ! Molecular weight of CFC11 (g/mol) - CFCL3
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REAL(KIND=JPRB) :: Z_AMC12                ! Molecular weight of CFC12 (g/mol) - CF2CL2
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REAL(KIND=JPRB) :: Z_AVGDRO               ! Avogadro's number (molecules/mole)
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REAL(KIND=JPRB) :: Z_GRAVIT               ! Gravitational acceleration (cm/sec2)
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! Atomic weights for conversion from mass to volume mixing ratios; these
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!  are the same values used in ECRT to assure accurate conversion to vmr
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data Z_AMD   /  28.970_JPRB    /
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data Z_AMW   /  18.0154_JPRB   /
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data Z_AMCO2 /  44.011_JPRB    /
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data Z_AMO   /  47.9982_JPRB   /
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data Z_AMCH4 /  16.043_JPRB    /
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data Z_AMN2O /  44.013_JPRB    /
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data Z_AMC11 / 137.3686_JPRB   /
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data Z_AMC12 / 120.9140_JPRB   /
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data Z_AVGDRO/ 6.02214E23_JPRB /
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data Z_GRAVIT/ 9.80665E02_JPRB /
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INTEGER(KIND=JPIM) :: IATM, IMOL, IXMAX, J1, J2, JAE, JB, JK, JL, I_L
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INTEGER(KIND=JPIM) :: I_NMOL, I_NXMOL
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REAL(KIND=JPRB) :: Z_AMM, ZCLDLY, ZCLEAR, ZCLOUD, ZEPSEC
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REAL(KIND=JPRB) :: ZHOOK_HANDLE
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!MPL/IM 20160915 on prend GES de phylmd
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#include "clesphys.h"
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! ***
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! *** mji
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! Initialize all molecular amounts and aerosol optical depths to zero here,
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! then pass ECRT amounts into RRTM arrays below.
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!      DATA ZWKL /MAXPRDW*0.0/
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!      DATA ZWX  /MAXPROD*0.0/
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!      DATA KREFLECT /0/
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! Activate cross section molecules:
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!     NXMOL     - number of cross-sections input by user
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!     IXINDX(I) - index of cross-section molecule corresponding to Ith
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!                 cross-section specified by user
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!                 = 0 -- not allowed in RRTM
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!                 = 1 -- CCL4
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!                 = 2 -- CFC11
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!                 = 3 -- CFC12
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!                 = 4 -- CFC22
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!      DATA KXMOL  /2/
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!      DATA KXINDX /0,2,3,0,31*0/
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!      IREFLECT=KREFLECT
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!      NXMOL=KXMOL
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IF (LHOOK) CALL DR_HOOK('RRTM_ECRT_140GP',0,ZHOOK_HANDLE)
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K_IREFLECT=0
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I_NXMOL=2
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DO J1=1,35
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! IXINDX(J1)=0
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  DO J2=1,KLEV
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    P_WKL(J1,J2)=0.0_JPRB
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  ENDDO
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ENDDO
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!IXINDX(2)=2
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!IXINDX(3)=3
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!     Set parameters needed for RRTM execution:
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IATM    = 0
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!      IXSECT  = 1
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!      NUMANGS = 0
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!      IOUT    = -1
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IXMAX   = 4
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!     Bands 6,7,8 are considered the 'window' and allowed to have a
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!     different surface emissivity (as in ECMWF).  Eli wrote this part....
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P_SEMISS(1)  = P_ZEMIS(K_IPLON)
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P_SEMISS(2)  = P_ZEMIS(K_IPLON)
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P_SEMISS(3)  = P_ZEMIS(K_IPLON)
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P_SEMISS(4)  = P_ZEMIS(K_IPLON)
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P_SEMISS(5)  = P_ZEMIS(K_IPLON)
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P_SEMISS(6)  = P_ZEMIW(K_IPLON)
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P_SEMISS(7)  = P_ZEMIW(K_IPLON)
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P_SEMISS(8)  = P_ZEMIW(K_IPLON)
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P_SEMISS(9)  = P_ZEMIS(K_IPLON)
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P_SEMISS(10) = P_ZEMIS(K_IPLON)
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P_SEMISS(11) = P_ZEMIS(K_IPLON)
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P_SEMISS(12) = P_ZEMIS(K_IPLON)
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P_SEMISS(13) = P_ZEMIS(K_IPLON)
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P_SEMISS(14) = P_ZEMIS(K_IPLON)
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P_SEMISS(15) = P_ZEMIS(K_IPLON)
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P_SEMISS(16) = P_ZEMIS(K_IPLON)
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!     Set surface temperature.
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P_TBOUND = pts(K_IPLON)
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!     Install ECRT arrays into RRTM arrays for pressure, temperature,
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!     and molecular amounts.  Pressures are converted from Pascals
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!     (ECRT) to mb (RRTM).  H2O, CO2, O3 and trace gas amounts are
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!     converted from mass mixing ratio to volume mixing ratio.  CO2
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!     converted with same dry air and CO2 molecular weights used in
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!     ECRT to assure correct conversion back to the proper CO2 vmr.
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!     The dry air column COLDRY (in molec/cm2) is calculated from
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!     the level pressures PZ (in mb) based on the hydrostatic equation
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!     and includes a correction to account for H2O in the layer.  The
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!     molecular weight of moist air (amm) is calculated for each layer.
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!     Note: RRTM levels count from bottom to top, while the ECRT input
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!     variables count from the top down and must be reversed here.
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K_NLAYERS = klev
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I_NMOL = 6
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PZ(0) = paph(K_IPLON,klev+1)/100._JPRB
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P_TZ(0) = pth(K_IPLON,klev+1)
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DO I_L = 1, KLEV
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  PAVEL(I_L) = pap(K_IPLON,KLEV-I_L+1)/100._JPRB
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  P_TAVEL(I_L) = pt(K_IPLON,KLEV-I_L+1)
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  PZ(I_L) = paph(K_IPLON,KLEV-I_L+1)/100._JPRB
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  P_TZ(I_L) = pth(K_IPLON,KLEV-I_L+1)
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  P_WKL(1,I_L) = pq(K_IPLON,KLEV-I_L+1)*Z_AMD/Z_AMW
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  P_WKL(2,I_L) = pcco2*Z_AMD/Z_AMCO2
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  P_WKL(3,I_L) = pozn(K_IPLON,KLEV-I_L+1)*Z_AMD/Z_AMO
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  P_WKL(4,I_L) = rn2o*Z_AMD/Z_AMN2O
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  P_WKL(6,I_L) = rch4*Z_AMD/Z_AMCH4
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  Z_AMM = (1-P_WKL(1,I_L))*Z_AMD + P_WKL(1,I_L)*Z_AMW
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  P_COLDRY(I_L) = (PZ(I_L-1)-PZ(I_L))*1.E3_JPRB*Z_AVGDRO/(Z_GRAVIT*Z_AMM*(1+P_WKL(1,I_L)))
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ENDDO
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!- Fill RRTM aerosol arrays with operational ECMWF aerosols,
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!  do the mixing and distribute over the 16 spectral intervals
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DO I_L=1,KLEV
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  JK=KLEV-I_L+1
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!       DO JAE=1,5
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  JAE=1
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  ZTAUAER(JAE) =&
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   & RAER(JAE,1)*PAER(K_IPLON,1,JK)+RAER(JAE,2)*PAER(K_IPLON,2,JK)&
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   & +RAER(JAE,3)*PAER(K_IPLON,3,JK)+RAER(JAE,4)*PAER(K_IPLON,4,JK)&
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   & +RAER(JAE,5)*PAER(K_IPLON,5,JK)+RAER(JAE,6)*PAER(K_IPLON,6,JK)
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  P_TAUAERL(I_L, 1)=ZTAUAER(1)
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  P_TAUAERL(I_L, 2)=ZTAUAER(1)
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  JAE=2
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  ZTAUAER(JAE) =&
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   & RAER(JAE,1)*PAER(K_IPLON,1,JK)+RAER(JAE,2)*PAER(K_IPLON,2,JK)&
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   & +RAER(JAE,3)*PAER(K_IPLON,3,JK)+RAER(JAE,4)*PAER(K_IPLON,4,JK)&
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   & +RAER(JAE,5)*PAER(K_IPLON,5,JK)+RAER(JAE,6)*PAER(K_IPLON,6,JK)
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  P_TAUAERL(I_L, 3)=ZTAUAER(2)
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  P_TAUAERL(I_L, 4)=ZTAUAER(2)
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  P_TAUAERL(I_L, 5)=ZTAUAER(2)
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  JAE=3
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  ZTAUAER(JAE) =&
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   & RAER(JAE,1)*PAER(K_IPLON,1,JK)+RAER(JAE,2)*PAER(K_IPLON,2,JK)&
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   & +RAER(JAE,3)*PAER(K_IPLON,3,JK)+RAER(JAE,4)*PAER(K_IPLON,4,JK)&
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   & +RAER(JAE,5)*PAER(K_IPLON,5,JK)+RAER(JAE,6)*PAER(K_IPLON,6,JK)
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  P_TAUAERL(I_L, 6)=ZTAUAER(3)
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  P_TAUAERL(I_L, 8)=ZTAUAER(3)
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  P_TAUAERL(I_L, 9)=ZTAUAER(3)
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  JAE=4
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  ZTAUAER(JAE) =&
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   & RAER(JAE,1)*PAER(K_IPLON,1,JK)+RAER(JAE,2)*PAER(K_IPLON,2,JK)&
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   & +RAER(JAE,3)*PAER(K_IPLON,3,JK)+RAER(JAE,4)*PAER(K_IPLON,4,JK)&
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   & +RAER(JAE,5)*PAER(K_IPLON,5,JK)+RAER(JAE,6)*PAER(K_IPLON,6,JK)
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  P_TAUAERL(I_L, 7)=ZTAUAER(4)
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  JAE=5
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  ZTAUAER(JAE) =&
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   & RAER(JAE,1)*PAER(K_IPLON,1,JK)+RAER(JAE,2)*PAER(K_IPLON,2,JK)&
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   & +RAER(JAE,3)*PAER(K_IPLON,3,JK)+RAER(JAE,4)*PAER(K_IPLON,4,JK)&
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   & +RAER(JAE,5)*PAER(K_IPLON,5,JK)+RAER(JAE,6)*PAER(K_IPLON,6,JK)
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!       END DO
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  P_TAUAERL(I_L,10)=ZTAUAER(5)
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  P_TAUAERL(I_L,11)=ZTAUAER(5)
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  P_TAUAERL(I_L,12)=ZTAUAER(5)
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  P_TAUAERL(I_L,13)=ZTAUAER(5)
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  P_TAUAERL(I_L,14)=ZTAUAER(5)
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  P_TAUAERL(I_L,15)=ZTAUAER(5)
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  P_TAUAERL(I_L,16)=ZTAUAER(5)
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ENDDO
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!--Use LW AOD from own Mie calculations (C. Kleinschmitt)
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DO I_L=1,KLEV
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  JK=KLEV-I_L+1
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  DO JAE=1, NLW
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    P_TAUAERL(I_L,JAE) = MAX( PTAU_LW(K_IPLON, JK, JAE), 1e-30 )
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  ENDDO
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ENDDO
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!--end C. Kleinschmitt
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DO J2=1,KLEV
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  DO J1=1,JPXSEC
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    P_WX(J1,J2)=0.0_JPRB
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  ENDDO
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ENDDO
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DO I_L = 1, KLEV
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!- Set cross section molecule amounts from ECRT; convert to vmr
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2791152
  P_WX(2,I_L) = rcfc11*Z_AMD/Z_AMC11
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  P_WX(3,I_L) = rcfc12*Z_AMD/Z_AMC12
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  P_WX(2,I_L) = P_COLDRY(I_L) * P_WX(2,I_L) * 1.E-20_JPRB
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  P_WX(3,I_L) = P_COLDRY(I_L) * P_WX(3,I_L) * 1.E-20_JPRB
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!- Here, all molecules in WKL and WX are in volume mixing ratio; convert to
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!  molec/cm2 based on COLDRY for use in RRTM
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19609632
  DO IMOL = 1, I_NMOL
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    P_WKL(IMOL,I_L) = P_COLDRY(I_L) * P_WKL(IMOL,I_L)
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  ENDDO
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! DO IX = 1,JPXSEC
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! IF (IXINDX(IX)  /=  0) THEN
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!     WX(IXINDX(IX),L) = COLDRY(L) * WX(IX,L) * 1.E-20_JPRB
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! ENDIF
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! END DO
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ENDDO
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!- Approximate treatment for various cloud overlaps
303
ZCLEAR=1.0_JPRB
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ZCLOUD=0.0_JPRB
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ZC1J(0)=0.0_JPRB
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ZEPSEC=1.E-03_JPRB
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JL=K_IPLON
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!++MODIFCODE
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71568
IF ((NOVLP == 1).OR.(NOVLP ==6).OR.(NOVLP ==8)) THEN
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!--MODIFCODE
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  DO JK=1,KLEV
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    IF (pcldf(JL,JK) > ZEPSEC) THEN
315
      ZCLDLY=pcldf(JL,JK)
316
      ZCLEAR=ZCLEAR &
317
       & *(1.0_JPRB-MAX( ZCLDLY , ZCLOUD ))&
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620301
       & /(1.0_JPRB-MIN( ZCLOUD , 1.0_JPRB-ZEPSEC ))
319
      ZCLOUD = ZCLDLY
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620301
      ZC1J(JK)= 1.0_JPRB - ZCLEAR
321
    ELSE
322
      ZCLDLY=0.0_JPRB
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      ZCLEAR=ZCLEAR &
324
       & *(1.0_JPRB-MAX( ZCLDLY , ZCLOUD ))&
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2170851
       & /(1.0_JPRB-MIN( ZCLOUD , 1.0_JPRB-ZEPSEC ))
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      ZCLOUD = ZCLDLY
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2170851
      ZC1J(JK)= 1.0_JPRB - ZCLEAR
328
    ENDIF
329
  ENDDO
330
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!++MODIFCODE
332
ELSEIF ((NOVLP == 2).OR.(NOVLP ==7)) THEN
333
!--MODIFCODE
334
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  DO JK=1,KLEV
336
    IF (pcldf(JL,JK) > ZEPSEC) THEN
337
      ZCLDLY=pcldf(JL,JK)
338
      ZCLOUD = MAX( ZCLDLY , ZCLOUD )
339
      ZC1J(JK) = ZCLOUD
340
    ELSE
341
      ZCLDLY=0.0_JPRB
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      ZCLOUD = MAX( ZCLDLY , ZCLOUD )
343
      ZC1J(JK) = ZCLOUD
344
    ENDIF
345
  ENDDO
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!++MODIFCODE
348
ELSEIF ((NOVLP == 3).OR.(NOVLP ==5)) THEN
349
!--MODIFCODE
350
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  DO JK=1,KLEV
352
    IF (pcldf(JL,JK) > ZEPSEC) THEN
353
      ZCLDLY=pcldf(JL,JK)
354
      ZCLEAR = ZCLEAR * (1.0_JPRB-ZCLDLY)
355
      ZCLOUD = 1.0_JPRB - ZCLEAR
356
      ZC1J(JK) = ZCLOUD
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    ELSE
358
      ZCLDLY=0.0_JPRB
359
      ZCLEAR = ZCLEAR * (1.0_JPRB-ZCLDLY)
360
      ZCLOUD = 1.0_JPRB - ZCLEAR
361
      ZC1J(JK) = ZCLOUD
362
    ENDIF
363
  ENDDO
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365
ELSEIF (NOVLP == 4) THEN
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367
ENDIF
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PTCLEAR=1.0_JPRB-ZC1J(KLEV)
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! Transfer cloud fraction and cloud optical depth to RRTM arrays;
371
! invert array index for pcldf to go from bottom to top for RRTM
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!- clear-sky column
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IF (PTCLEAR  >  1.0_JPRB-ZEPSEC) THEN
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2151
  KCLD=0
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86040
  DO I_L = 1, KLEV
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86040
    P_CLDFRAC(I_L) = 0.0_JPRB
378
  ENDDO
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36567
  DO JB=1,JPBAND
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1378791
    DO I_L=1,KLEV
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1376640
      P_TAUCLD(I_L,JB) = 0.0_JPRB
382
    ENDDO
383
  ENDDO
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385
ELSE
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387
!- cloudy column
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!   The diffusivity factor (Savijarvi, 1997) on the cloud optical
389
!   thickness TAUCLD has already been applied in RADLSW
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391
69417
  KCLD=1
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2776680
  DO I_L=1,KLEV
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    P_CLDFRAC(I_L) = pcldf(K_IPLON,I_L)
394
  ENDDO
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1180089
  DO JB=1,JPBAND
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44496297
    DO I_L=1,KLEV
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44426880
      P_TAUCLD(I_L,JB) = ptaucld(K_IPLON,I_L,JB)
398
    ENDDO
399
  ENDDO
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401
ENDIF
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!     ------------------------------------------------------------------
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IF (LHOOK) CALL DR_HOOK('RRTM_ECRT_140GP',1,ZHOOK_HANDLE)
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END SUBROUTINE RRTM_ECRT_140GP