source: trunk/LMDZ.VENUS/libf/phyvenus/load_ksi.F @ 3094

      SUBROUTINE load_ksi(ksive)
      
      use dimphy
      IMPLICIT none

#include "YOMCST.h"
#include "comcstVE.h"
C
C     ------------------------------------------------------------------
C
C     PURPOSE.
C     --------
C
c     This routine loads the longwave matrix of factors Ksi
c     
c     The Ksi matrixes have been computed by Vincent Eymet
C
C     AUTHOR.
C     -------
C        Sebastien Lebonnois
C
C     MODIFICATIONS.
C     --------------
C        
c   New ksi matrix: possibility of different cloud model fct of lat   05/2014
C     ------------------------------------------------------------------
C
C* ARGUMENTS:
C
c inputs
      real   psurf(klon)           ! Surface pressure
c outputs
      real   ksive(0:klev+1,0:klev+1,nnuve,nbmat)  ! ksi matrixes in Vincent's file

c local variables
      integer i,j,isza,ips,band,pve,sve,nlve
      integer lat,Nb,m,mat
      character*9 tmp1
      character*100 file
      CHARACTER*2 str2
      CHARACTER*3 str3
      CHARACTER*10 format_lect 
      real   lambda(nnuve)            ! wavelenght in table (mu->m, middle of interval)
      real   lambdamin(nnuve),lambdamax(nnuve) ! in microns
      real   dlambda                  ! in microns 
      logical upper

      nlve = klev

cc      GG modif below 
c----------------------------------
c   Initialisation of values to 0 
c     (for all vertical levels)
c----------------------------------

      ksive(0:klev+1,0:klev+1,1:nnuve,1:nbmat) = 0.0

c ------------------------
c Loading the ksi file
c ------------------------

      file = "ksi_global.txt"
      open(10,file=file)
      
      read(10,*)
      read(10,*) nlatve
      read(10,*)

      write(*,*) 'This is subroutine load_ksi'
      write(*,*) 'Nb of lat bands:',nlatve
      
      do lat=1,nlatve
        read(10,*) !line for lat range
        read(10,*) indexve(lat)
        read(10,*) nbpsve(lat)
        read(10,*)
        read(10,*) nbszave(lat)
        read(10,*)
        
        do isza=1,nbszave(lat)
          do ips=1,nbpsve(lat)
          
        read(10,*) (tmp1,j=1,3),mat    !line for matrix number
        read(10,*) (tmp1,j=1,2),pve
        psurfve(ips,lat) = pve*1.e5    ! pve in bar, psurfve in Pa
        read(10,*) (tmp1,j=1,3),sve 
        szave(isza,lat) = cos(sve*RPI/180.) ! conversion in mu0
        read(10,*)
        read(10,*) m,Nb
CC vertical axis check
        upper=.false.
cc the number of levels read for the matrix (m) should be the number of levels of the GCM (nlve=klev)
        if (m.ne.nlve) then
CC When GCM axis has more levels than the matrix, we must be in the case
cc with upper atmosphere, ie matrix limited to 78 levels and upper levels set to zero
cc otherwise there is a problem
         if ((m.eq.78).and.(nlve.gt.78)) then
          upper=.true.
         else
          write(*,*) 'This is subroutine load_ksi'
          print*,'Dimension problem between ksi.txt and nlve'
          print*,'N levels = ',m,nlve
          stop
         endif
        endif
cc wavelength check
        if (Nb.ne.nnuve) then
         write(*,*) 'This is subroutine load_ksi'
         print*,'Dimension problem between ksi.txt and nnuve'
         print*,'N freq = ',Nb,nnuve
         stop
        endif
c     Now reading ksi matrix index "mat"
        if ((m+2).ge.100) then
          write(str3,'(i3.3)') m+2
          format_lect='('//str3//'e17.9)'
        else
          write(str2,'(i2.2)') m+2
          format_lect='('//str2//'e17.9)'
        endif
        do band=1,Nb
         read(10,*) lambdamin(band),lambdamax(band)
         do i=0,m+1
            read(10,format_lect) (ksive(i,j,band,mat),j=0,m+1) ! no unit
         enddo                  ! i
cc case upper atmosphere: the level for space (m+1) should be raised to nlve+1
         if (upper) then
           do i=0,m
             ksive(i,klev+1,band,mat)=ksive(i,m+1,band,mat)
             ksive(i,m+1,band,mat)=0.
           enddo
             ksive(klev+1,:,band,mat)=ksive(m+1,:,band,mat)
             ksive(m+1,:,band,mat)=0.
         endif
        enddo                     ! band
c       print*,"Matrice ",mat," lue"
c       print*,"   psurf=",psurfve(ips,lat)," bars"
        if (mat+1.gt.nbmat) then
         write(*,*) 'This is subroutine load_ksi'
         print*,'Dimension problem between ksi.txt and nbmat'
         print*,'(max number of matrixes)'
         print*,'nbmat (in comcstVE.h) should be raised'
         stop
        endif

          enddo    ! ips
        enddo      ! isza
      enddo        ! lat
      
      write(*,*) 'Total nb of matrixes:',mat
      
      close(10)

c central wavelength and wavelength width
      do band=1,nnuve
         lambda(band)=(lambdamin(band)+lambdamax(band))/2.*1.e-6   ! in m
         dlambda     =(lambdamax(band)-lambdamin(band))            ! in microns
c        print*,band,lambdamin(band),dlambda,lambdamax(band)

c sign convention for ksi,
c and taking into account the wavelength width (in microns):
         do mat=1,nbmat
         do i=0,nlve+1
           do j=0,nlve+1
              ksive(i,j,band,mat) = +ksive(i,j,band,mat)*dlambda    ! in µm
           enddo
         enddo
         enddo
c computing coeff al and bl for Planck luminance 
         al(band) = 2.*RHPLA*RCLUM*RCLUM/(lambda(band))**5.
c in W/m²/m
c We need W/m²/µm :
     .                * 1.e-6
         bl(band) = RHPLA*RCLUM/(RKBOL*lambda(band))
      enddo
      
      print*,"LOAD_KSI OK"

      return
      end