Ignore:
Timestamp:
Sep 5, 2012, 8:32:32 PM (12 years ago)
Author:
jleconte
Message:

05/09/2012 == JL

  • Correction of the calculation of the solar longitude in tlocked case.

-Can now handle any prograde resonance with nres=omega_rot/omega_orb.
-Sun now goes westward for the standard 2:1 case, as expected.

  • In the gray case, the separation between kappa_IR and VI is now set by

wave number, independently of the usual IR/VISIBLE calculation separation.
i.e. kappa_IR can be used in the calculation of the downward stellar flux

if the wavenumber in the band is low enough and vice versa.

  • In ave_stelspec, stellar flux averaging has been generalized to incorporate

very red/blue stellar spectra (great care must however be taken of the band
limit used for the corralated k distributions).

-Brown dwarf spectra from Allard et al. have been added.
-Any Black body temperature can now be used.


File:
1 edited

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  • trunk/LMDZ.GENERIC/README

    r751 r773  
    750750- Bug fix in physiq : the size of OLR_nu is L_NSPECTI and not L_NSPECTV
    751751- A more robust aerosol_mod + iniaerosol : problems with ifort+parallel solved, while still OK with other compilers and seq runs.
     752
     753== 05/09/2012 == JL
     754- Correction of the calculation of the solar longitude in tlocked case.
     755    -Can now handle any prograde resonance with nres=omega_rot/omega_orb.
     756    -Sun now goes westward for the standard 2:1 case, as expected.
     757- In the gray case, the separation between kappa_IR and VI is now set by
     758    wave number, independently of the usual IR/VISIBLE calculation separation.
     759    i.e. kappa_IR can be used in the calculation of the downward stellar flux
     760      if the wavenumber in the band is low enough and vice versa.
     761- In ave_stelspec, stellar flux averaging has been generalized to incorporate
     762    very red/blue stellar spectra (great care must however be taken of the band
     763    limit used for the corralated k distributions).
     764     -Brown dwarf spectra from Allard et al. have been added.
     765     -Any Black body temperature can now be used.
     766
     767 
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