subroutine calc_rayleigh !================================================================== ! ! Purpose ! ------- ! Average the Rayleigh scattering in each band, weighting the ! average by the blackbody function at temperature tstellar. ! Works for an arbitrary mix of gases (currently CO2, N2 and ! H2 are possible). ! ! Authors ! ------- ! Robin Wordsworth (2010) ! ! Called by ! --------- ! setspv.F ! ! Calls ! ----- ! none ! !================================================================== use radinc_h, only: L_NSPECTV use radcommon_h, only: WAVEV, BWNV, DWNV, tstellar, tauray, scalep use gases_h implicit none #include "comcstfi.h" #include "callkeys.h" real*8 wl integer N,Nfine,ifine,igas parameter(Nfine=500.0) real*8 :: P0 = 9.423D+6 ! Rayleigh scattering reference pressure in pascals. logical typeknown real*8 tauvar,tausum,tauwei,bwidth,bstart double precision df real*8 tauconsti(ngasmx) real*8 tauvari(ngasmx) integer icantbewrong ! tau0/p0=tau/p (Hansen 1974) ! Then calculate tau0 = (8*pi^3*p_1atm)/(3*N0^2) * 4*delta^2/(g*mugaz*lambda^4) ! where delta=n-1 and N0 is an amagat typeknown=.false. do igas=1,ngasmx if(igas.eq.vgas)then print*,'Ignoring ',gnom(igas),' in Rayleigh scattering '// & 'as it is variable.' elseif(gfrac(igas).lt.5.e-2)then print*,'Ignoring ',gnom(igas),' in Rayleigh scattering '// & 'as its mixing ratio is less than 0.05.' ! ignore variable gas in Rayleigh calculation ! ignore gases of mixing ratio < 0.05 in Rayleigh calculation tauconsti(igas) = 0.0 else if(gnom(igas).eq.'CO2')then tauconsti(igas) = (8.7/g)*1.527*scalep/P0 elseif(gnom(igas).eq.'N2_')then tauconsti(igas) = (9.81/g)*8.569E-3*scalep/(P0/93.0) elseif(gnom(igas).eq.'H2O')then tauconsti(igas) = (10.0/g)*9.22E-3*scalep/101325.0 elseif(gnom(igas).eq.'H2_')then tauconsti(igas) = (10.0/g)*0.0241*scalep/101325.0 !tauconsti(igas) = (10.0/g)*0.0487*scalep/(101325.0) ! uses n=1.000132 from Optics, Fourth Edition. ! was out by a factor 2! elseif(gnom(igas).eq.'He_')then print*,'Helium not ready yet!' tauconsti(igas) = 0.0 call abort else print*,'Error in calc_rayleigh: Gas species not recognised!' call abort endif if(gfrac(igas).eq.1.0)then print*,'Rayleigh scattering is for a pure ',gnom(igas),' atmosphere.' typeknown=.true. endif endif enddo if(.not.typeknown)then print*,'Rayleigh scattering is for a mixed gas atmosphere.' typeknown=.true. endif do N=1,L_NSPECTV tausum = 0.0 tauwei = 0.0 bstart = 10000.0/BWNV(N+1) bwidth = (10000.0/BWNV(N)) - (10000.0/BWNV(N+1)) do ifine=1,Nfine wl=bstart+dble(ifine)*bwidth/Nfine tauvar=0.0 do igas=1,ngasmx if((igas.eq.vgas).or.(gfrac(igas).lt.5.e-2))then ! ignore variable gas in Rayleigh calculation ! ignore gases of mixing ratio < 0.05 in Rayleigh calculation tauvari(igas) = 0.0 else if(gnom(igas).eq.'CO2')then tauvari(igas) = (1.0+0.013/wl**2)/wl**4 elseif(gnom(igas).eq.'N2_')then tauvari(igas) = (1.0+0.0113/wl**2+0.00013/wl**4)/wl**4 elseif(gnom(igas).eq.'H2O')then tauvari(igas) = 1.0/wl**4 ! to be improved... elseif(gnom(igas).eq.'H2_')then tauvari(igas) = 1.0/wl**4 elseif(gnom(igas).eq.'He_')then print*,'Helium not ready yet!' tauvari(igas) = 0.0 else print*,'Error in calc_rayleigh: Gas species not recognised!' call abort endif endif tauvar=tauvar+tauconsti(igas)*tauvari(igas)*gfrac(igas) enddo call blackl(dble(wl*1e-6),dble(tstellar),df) df=df*bwidth/Nfine tauwei=tauwei+df tausum=tausum+tauvar*df enddo TAURAY(N)=tausum/tauwei ! we multiply by scalep here (100) because plev, which is used in optcv, ! is in units of mBar, so we need to convert. end do IF (L_NSPECTV > 6) THEN icantbewrong = L_NSPECTV-6 print*,'At 1 atm and lambda = ',WAVEV(icantbewrong),' um' print*,'tau_R = ',TAURAY(icantbewrong)*1013.25 print*,'sig_R = ',TAURAY(icantbewrong)*g*mugaz*1.67e-27*100, & 'cm^2 molecule^-1' ENDIF end subroutine calc_rayleigh