Ignore:
Timestamp:
Jun 21, 2013, 1:07:34 AM (12 years ago)
Author:
aslmd
Message:

LMDZ.GENERIC. Updated saturn 1D files. Added comments around the gluxi problem (will be further investigated). removed abort because Helium rayleigh scattering is missing

Location:
trunk/LMDZ.GENERIC/libf/phystd
Files:
2 edited

Legend:

Unmodified
Added
Removed
  • trunk/LMDZ.GENERIC/libf/phystd/calc_rayleigh.F90

    r869 r995  
    7777               print*,'Helium not ready yet!'
    7878               tauconsti(igas) = 0.0
    79                call abort
     79               !call abort
    8080            else
    8181               print*,'Error in calc_rayleigh: Gas species not recognised!'
  • trunk/LMDZ.GENERIC/libf/phystd/gfluxi.F

    r961 r995  
    101101      LAMDA(L) = ALPHA(L)*(1.0D0-W0(L)*COSBAR(L))/UBARI
    102102
     103      ! Tsurf is used for 1st layer source function
     104      ! -- same results for most thin atmospheres
     105      ! -- and stabilizes integrations
    103106      NT    = int(TLEV(2*L+1)*NTfac) - NTstar+1
     107
     108      !! For deep, opaque, thick first layers (e.g. Saturn)
     109      !! what is below works much better, not unstable, ...
     110      !! ... and actually fully accurate because 1st layer temp (JL)
     111      !NT    = int(TLEV(2*L)*NTfac) - NTstar+1
     112      !! (or this one yields same results
     113      !NT    = int( (TLEV(2*L)+TLEV(2*L+1))*0.5*NTfac ) - NTstar+1
     114
    104115      NT2   = int(TLEV(2*L)*NTfac)   - NTstar+1
    105116      B1(L) = (PLANCKIR(NW,NT)-PLANCKIR(NW,NT2))/DTAU(L)
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