Ignore:
Timestamp:
Sep 7, 2021, 9:57:37 AM (3 years ago)
Author:
abierjon
Message:

Mars GCM:
simu_MCS.F90 : now computes the column-integrated dust optical depths of the MCS and GCM files
(between levels with no missing values in both files, which vary with space and time) and outputs
the ratio tau_GCM/tau_MCS to be used to normalize the GCM dust opacity profiles when comparing to MCSake simu_MCS.F90 compatible with DYNAMICO lon-lat output files, with a check on the latitude array order when doing the interpolation

AB

File:
1 edited

Legend:

Unmodified
Added
Removed
  • trunk/LMDZ.MARS/README

    r2554 r2558  
    34383438Make NO and O2 Nightglow emissions computations more flexible (reaction index
    34393439 no longer hard coded in photochemistry.F90).
     3440 
     3441== 07/09/2021 == AB
     3442simu_MCS.F90 : now computes the column-integrated dust optical depths of the MCS and GCM files
     3443(between levels with no missing values in both files, which vary with space and time) and outputs
     3444the ratio tau_GCM/tau_MCS to be used to normalize the GCM dust opacity profiles when comparing to MCS
Note: See TracChangeset for help on using the changeset viewer.