source: trunk/LMDZ.GENERIC/libf/phystd/calc_rayleigh.F90 @ 649

Last change on this file since 649 was 471, checked in by aslmd, 13 years ago

LMDZ.GENERIC

13/12/2011 == AS

  • Same spirit as previous commit, but for ngasmx which is now read in gases.def -- before arrays w/ dim ngasmx are allocated dynamically
  • Allocation is done in su_gases.F90 which is called in inifis
  • Outside su_gases.F90, very few modifications to the code : the new module "gases_h.F90" simply replaces the old common "gases.h" !
  • Compiles fine. Tested with debugging options through pgdbg. Runs fine. Exact same results in Early Mars test case.
File size: 4.8 KB
RevLine 
[135]1      subroutine calc_rayleigh
2
3!==================================================================
4!     
5!     Purpose
6!     -------
7!     Average the Rayleigh scattering in each band, weighting the
8!     average by the blackbody function at temperature tstellar.
[253]9!     Works for an arbitrary mix of gases (currently CO2, N2 and
10!     H2 are possible).
[135]11!     
12!     Authors
13!     -------
14!     Robin Wordsworth (2010)
15!
16!     Called by
17!     ---------
18!     setspv.F
19!     
20!     Calls
21!     -----
22!     none
23!     
24!==================================================================
25
26      use radinc_h, only: L_NSPECTV
[253]27      use radcommon_h, only: WAVEV, BWNV, DWNV, tstellar, tauray, scalep
[471]28      use gases_h
[135]29
30      implicit none
31
32#include "comcstfi.h"
[253]33#include "callkeys.h"
[135]34
35      real*8 wl
[253]36      integer N,Nfine,ifine,igas
[135]37      parameter(Nfine=500.0)
38      real*8 :: P0 = 9.423D+6   ! Rayleigh scattering reference pressure in pascals.   
39
[253]40      logical typeknown
41      real*8 tauvar,tausum,tauwei,bwidth,bstart
[135]42      double precision df
43
[253]44      real*8 tauconsti(ngasmx)
45      real*8 tauvari(ngasmx)
[135]46
[253]47      ! tau0/p0=tau/p (Hansen 1974)
[305]48      ! Then calculate tau0 = (8*pi^3*p_1atm)/(3*N0^2) * 4*delta^2/(g*mugaz*lambda^4)
49      ! where delta=n-1 and N0 is an amagat
[253]50
51      typeknown=.false.
52      do igas=1,ngasmx
53         if(igas.eq.vgas)then
54            print*,'Ignoring ',gnom(igas),' in Rayleigh scattering '// &
55            'as it is variable.'
56         elseif(gfrac(igas).lt.5.e-2)then
57            print*,'Ignoring ',gnom(igas),' in Rayleigh scattering '// &
58            'as its mixing ratio is less than 0.05.'
59            ! ignore variable gas in Rayleigh calculation
[305]60            ! ignore gases of mixing ratio < 0.05 in Rayleigh calculation
[253]61            tauconsti(igas) = 0.0
[135]62         else
[253]63            if(gnom(igas).eq.'CO2')then
64               tauconsti(igas) = (8.7/g)*1.527*scalep/P0
65            elseif(gnom(igas).eq.'N2_')then
66               tauconsti(igas) = (9.81/g)*8.569E-3*scalep/(P0/93.0)
[305]67            elseif(gnom(igas).eq.'H2O')then
68               tauconsti(igas) = (10.0/g)*9.22E-3*scalep/101325.0
[253]69            elseif(gnom(igas).eq.'H2_')then
[305]70               tauconsti(igas) = (10.0/g)*0.0241*scalep/101325.0
71               !tauconsti(igas) = (10.0/g)*0.0487*scalep/(101325.0)
[253]72               ! uses n=1.000132 from Optics, Fourth Edition.
[305]73               ! was out by a factor 2!
[253]74            elseif(gnom(igas).eq.'He_')then
75               print*,'Helium not ready yet!'
76            else
77               print*,'Error in calc_rayleigh: Gas species not recognised!'
78               call abort
79            endif
80
81            if(gfrac(igas).eq.1.0)then
82               print*,'Rayleigh scattering is for a pure ',gnom(igas),' atmosphere.'
83               typeknown=.true.
84            endif
85
[135]86         endif
[253]87      enddo
88
89      if(.not.typeknown)then
90         print*,'Rayleigh scattering is for a mixed gas atmosphere.'
91         typeknown=.true.
[135]92      endif
[253]93
[135]94 
95      do N=1,L_NSPECTV
96         
[253]97         tausum = 0.0
98         tauwei = 0.0
99         bstart = 10000.0/BWNV(N+1)
100         bwidth = (10000.0/BWNV(N)) - (10000.0/BWNV(N+1))
101         do ifine=1,Nfine
102            wl=bstart+dble(ifine)*bwidth/Nfine
[135]103
[253]104            tauvar=0.0
105            do igas=1,ngasmx
106               if((igas.eq.vgas).or.(gfrac(igas).lt.5.e-2))then
107                  ! ignore variable gas in Rayleigh calculation
[305]108                  ! ignore gases of mixing ratio < 0.05 in Rayleigh calculation
[253]109                  tauvari(igas)   = 0.0
110               else
111                  if(gnom(igas).eq.'CO2')then
112                     tauvari(igas) = (1.0+0.013/wl**2)/wl**4
113                  elseif(gnom(igas).eq.'N2_')then
114                     tauvari(igas) = (1.0+0.0113/wl**2+0.00013/wl**4)/wl**4
[305]115                  elseif(gnom(igas).eq.'H2O')then
116                     tauvari(igas) = 1.0/wl**4 ! to be improved...
[253]117                  elseif(gnom(igas).eq.'H2_')then
[305]118                     tauvari(igas) = 1.0/wl**4
[253]119                  else
120                     print*,'Error in calc_rayleigh: Gas species not recognised!'
121                     call abort
122                  endif
123               endif
[135]124
[253]125               tauvar=tauvar+tauconsti(igas)*tauvari(igas)*gfrac(igas)
126
[135]127            enddo
128
[253]129            call blackl(dble(wl*1e-6),dble(tstellar),df)
130            df=df*bwidth/Nfine
131            tauwei=tauwei+df
132            tausum=tausum+tauvar*df
133         
134         enddo
135         TAURAY(N)=tausum/tauwei
[135]136         ! we multiply by scalep here (100) because plev, which is used in optcv,
137         ! is in units of mBar, so we need to convert.
[253]138
[135]139      end do
140
[305]141      print*,'At 1 atm and lambda = ',WAVEV(L_NSPECTV-6),' um'
142      print*,'tau_R = ',TAURAY(L_NSPECTV-6)*1013.25
143      print*,'sig_R = ',TAURAY(L_NSPECTV-6)*g*mugaz*1.67e-27*100, &
144             'cm^2 molecule^-1'
[253]145
[135]146    end subroutine calc_rayleigh
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