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Timestamp:
Nov 15, 2018, 10:25:09 AM (6 years ago)
Author:
emillour
Message:

Mars GCM:
Modifications to use the parametrized photoabsorbtion coefficients;
a first step towards implementing ionospheric chemistry in the new
chemical solver:

  • change in species indexes in chemthermos.F90, paramfoto_compact.F, hrtherm.F and euvheat.F90
  • calchim.F90: added a variable in call to photochemistry
  • photochemistry.F90: added calls to jthermcalc_e107 and phdisrate, with an additionlal flag, jparam (.false. by default). The computed photodissociation coefficents are sent to v_phot, which is used in the chemistry. Thus concentrations computed in chimtogcm are now done over all atmospheric layers.

FGG

File:
1 edited

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  • trunk/LMDZ.MARS/README

    r2023 r2042  
    26592659- Fix writediagsoil so that it also works in parallel.
    26602660
    2661 
     2661== 15/11/2018 == FGG
     2662Modifications to use the parametrized photoabsorbtion coefficients;
     2663a first step towards implementing ionospheric chemistry in the new
     2664chemical solver:
     2665- change in species indexes in chemthermos.F90, paramfoto_compact.F,
     2666  hrtherm.F and euvheat.F90
     2667- calchim.F90: added a variable in call to photochemistry
     2668- photochemistry.F90: added calls to jthermcalc_e107 and phdisrate,
     2669  with an additionlal flag, jparam (.false. by default). The
     2670  computed photodissociation coefficents are sent to v_phot, which
     2671  is used in the chemistry. Thus concentrations computed in
     2672  chimtogcm are now done over all atmospheric layers.
     2673
     2674et jthermcalc.F
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