source: trunk/LMDZ.MARS/libf/phymars/swmain.F @ 1972

      SUBROUTINE SWMAIN ( KDLON, KFLEV,
     $                PCST, albedo,
     $                PRMU0, PDP, PPLEV, aerosol,PFRACT,
     $                PHEAT, PFLUXD,PFLUXU,
     &                QVISsQREF3d,omegaVIS3d,gVIS3d)

      use dimradmars_mod, only: ndlo2, ndlon, nflev, 
     &                          nsun,naerkind
      use yomlw_h, only: nlaylte, gcp
      IMPLICIT NONE
      
#include "callkeys.h"
c     
c     PURPOSE.
c     --------
c     
c     This routine computes the shortwave (solar wavelength)
c     radiation fluxes in two spectral intervals 
c     and heating rate on the first "nlaylte" layers.
C     
c     Francois Forget (2000), adapted from 
C     Fouquart and Bonnel's ECMWF program
c 
C     IMPLICIT ARGUMENTS :
C     --------------------
C     
C     ==== INPUTS ===
c
c    KDLON :  number of horizontal grid points
c    PCST  :  Solar constant on Mars (W.m-2)
c    albedo   hemispheric surface albedo
c                         albedo (i,1) : mean albedo for solar band#1
c                                        (see below)
c                         albedo (i,2) : mean albedo for solar band#2
c                                        (see below)
c    PRMU0 :         cos of solar zenith angle (=1 when sun at zenith)
c    PDP :           Layer thickness (Pa)
c    PPLEV           pressure (Pa) at boundaries of each layer 
c   aerosol               aerosol extinction optical depth
c                         at reference wavelength "longrefvis" set
c                         in dimradmars_mod , in each layer, for one of
c                         the "naerkind" kind of aerosol optical properties.
c    Pfract :        day fraction of the time interval
c                          =1 during the full day ; =0 during the night
c    QVISsQREF3d,omegaVIS3d,gVIS3d Aerosol optical properties
c
C     ==== OUTPUTS ===
c    PHEAT :         Heating rate (K/s)
c    PFLUXD :        SW downward flux at boundaries of each layer (W.m-2)
c    PFLUXU :        SW upward flux at boundaries of each layer (W.m-2)
C     
C     ----------
C     
C-----------------------------------------------------------------------
C     
C     
C-----------------------------------------------------------------------
C     
C     ARGUMENTS
C     ---------
      
      INTEGER KDLON, KFLEV
      REAL ZPSOL(NDLO2), aerosol(NDLO2,KFLEV,naerkind),PRMU0(NDLO2)
      real PCST
      REAL albedo(NDLO2,2)
      REAL PDP(NDLO2,KFLEV)
      REAL PPLEV(NDLO2,KFLEV+1)
      REAL PHEAT(NDLO2,KFLEV)
      REAL PFRACT(NDLO2)
      real PFLUXD(NDLON,NFLEV+1,2)
      real PFLUXU(NDLON,NFLEV+1,2)
      REAL :: QVISsQREF3d(NDLO2,KFLEV,nsun,naerkind)
      REAL :: omegaVIS3d(NDLO2,KFLEV,nsun,naerkind)
      REAL :: gVIS3d(NDLO2,KFLEV,nsun,naerkind)
      
C     LOCAL ARRAYS
C     ------------
      
      REAL ZDSIG(NDLON,NFLEV), ZFACT(NDLON)
     S     ,  ZFD(NDLON,NFLEV+1)
     S     ,  ZFU(NDLON,NFLEV+1)
     S     ,  ZRMU(NDLON), ZSEC(NDLON)
     S     ,  ZUD(NDLON,3,NFLEV+1), ZUM(NDLON,NFLEV+1)
      REAL ZSIGN(NDLON),  ZSIGO(NDLON)

c following line has been changed, kflev--->nflev (to avoid error message 
c when compiling on NASA Ames Sun)
      REAL ZFDOWN(NDLO2,NFLEV+1),ZFUP(NDLO2,NFLEV+1)

      integer jl, jk, jkp1, jkl
      integer INU 
      real  zdfnet

C     ------------------------------------------------------------------
C     Initializations :
C     ------------------------------------------------------------------

c     Incident Solar flux and corrected angle in the atmosphere 
c     ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
      DO JL = 1 , KDLON
c        Incident Flux at the top of the atmosphere
         ZFACT(JL)= PRMU0(JL) * PCST * PFRACT(JL)

c        Cos of solar zenith angle CORRECTED for high zenith angle
       if (PRMU0(JL).GT.0) then
         ZRMU(JL)=SQRT(1224.* PRMU0(JL) * PRMU0(JL) + 1.) / 35.
       else
         ZRMU(JL)= 1. / 35.
       endif
         ZSEC(JL)=1./ZRMU(JL)
      END DO

c     Calcul of ZDSIG  (thickness of layers in sigma coordinates)
c     ~~~~~~~~~~~~~~~
      DO JL = 1 , KDLON
         ZSIGO(JL) = 1.0
         ZPSOL(JL) = PPLEV(JL,1)
      END DO
      DO JK = 1 , nlaylte
         JKP1 = JK + 1
         JKL = nlaylte+1 - JK
         DO  JL = 1 , KDLON
            ZSIGN(JL) = PPLEV(JL,JKP1) / PPLEV(JL,1)
            ZDSIG(JL,JK) = ZSIGO(JL) - ZSIGN(JL)
            ZSIGO(JL) = ZSIGN(JL)
         END DO
      END DO

C------------------------------------------------------------------
C          LOOP ON SPECTRAL INTERVAL in solar spectrum
C------------------------------------------------------------------
c  2 spectral interval in solar spectrum :
c  - INU=1: between wavelength "long1vis" and "long2vis" set in dimradmars_mod
c  - INU=2: between wavelength "long2vis" and "long3vis" set in dimradmars_mod

      DO INU = 1,2

! NB: swrtype is set in callkeys.h
        if (swrtype.eq.1) then ! Fouquart
          CALL SWR_FOUQUART( KDLON, kflev, INU
     &     ,  aerosol,QVISsQREF3d,omegaVIS3d,gVIS3d
     &     ,  albedo,ZDSIG,ZPSOL,ZRMU,ZSEC
     &     ,  ZFD,ZFU )
        else
          if (swrtype.eq.2) then ! Toon
            CALL SWR_TOON( KDLON, kflev, INU
     &       ,  aerosol,QVISsQREF3d,omegaVIS3d,gVIS3d
     &       ,  albedo,ZDSIG,ZPSOL,ZRMU,ZSEC
     &       ,  ZFD,ZFU )
          else
            write(*,*) "swmain: invalid swrtype value !!"
            stop
          endif ! of if (swrtype.eq.2)
        endif ! of if (swrtype.eq.1)
        
         DO JK = 1 , nlaylte+1
            DO  JL = 1 , KDLON
              PFLUXD(JL,JK,INU)=ZFD(JL,JK)*ZFACT(JL)
              PFLUXU(JL,JK,INU)=ZFU(JL,JK)*ZFACT(JL)
            END DO
         END DO
      END DO ! of DO INU=1,2

C     ------------------------------------------------------
C     HEATING RATES
C     ------------------------------------------------------

      DO JK = 1 , nlaylte+1
         DO  JL = 1 , KDLON
c           wavelength integrated flux at every level:
            ZFUP(JL,JK)= (PFLUXU(JL,JK,1)+ PFLUXU(JL,JK,2))
            ZFDOWN(JL,JK)= (PFLUXD(JL,JK,1)+ PFLUXD(JL,JK,2))
         END DO
      END DO
     
      DO JK = 1 , nlaylte
         DO  JL = 1 , KDLON
            ZDFNET = ZFUP (JL,JK  ) - ZFDOWN(JL,JK  )
     S              -ZFUP (JL,JK+1) + ZFDOWN(JL,JK+1)
c           Heating rate
            PHEAT(JL,JK) = gcp * ZDFNET / PDP(JL,JK)
         END DO
      END DO

      RETURN
      END