Changes between Version 52 and Version 53 of ArchiveReport


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Timestamp:
Apr 30, 2021, 10:50:15 AM (4 years ago)
Author:
cmathe
Comment:

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  • ArchiveReport

    v52 v53  
    11= Archive of POULDP reports =
    22
     3'''29^th^ April 2021'''
     4{{{
     5
     6Duration: 1h30mn
     7
     8Participants: Lucas, Joseph, Siteng, Ehouarn, Romain, Thomas, Francisco, Antoine, Francois, Antony
     9Margaux, Aymeric, Christophe
     10
     11Recent commits: https://trac.lmd.jussieu.fr/Planeto/log
     12==============
     13- r2502: set icelocationmode=4 as default mode (set watercaptags as before) in surfini
     14- r2505: code clean-up (remove obsolete files in LMDZ.MARS/libf/dynphy_lonlat)
     15- r2507: modifications in the calendar values stored in restart files for 1+1=2
     16- r2508: separating water ice deposit albedo cases between "cap" and "frost"
     17
     18Recent tickets: https://trac.lmd.jussieu.fr/Planeto/report/1
     19==============
     20- None
     21
     22Wiki updates: https://trac.lmd.jussieu.fr/Planeto/wiki
     23============
     24- None
     25
     26Ongoing discussions:
     27===================
     28
     29* Brutal drying up in the thermosphere issue: (Francisco, Margaux, Francois)
     30Francisco found the problem comes from a drastic 1.e-8 threshold correction in waterclouds
     31Strong improvement in the upper atmosphere when setting this threshold to 1.e-12
     32Francois did some tests with 1.e-16 => does influence the polar hood, but the later is
     33quite variable from a week to the next
     34It also makes sens for HDO computations to lower this threshold.
     35=> All agree we should lower the threshold to 1.e-16
     36=> Francois will check saturation at 90K to target the value
     37
     38* Crash with unexpected unrealistic HDO ratio: (Jean-Yves, Margaux, Ehouarn)
     39HDO_ice ratio of 4000 from the dynamics
     40Problem identified (with isotopes) to comes from the dynamics
     41
     42* Comparing GCM runs with TIRVIM (& MCS): (Antoine, Sandrine, Siteng)
     43
     44* Dynamico-Mars:
     45- what time to set when calling the physics from dynamico?
     46- what calendar setup to use in XIOS? Still needs to be checked due to restarts, etc.
     47
     48Christophe:
     49- someone should make a utility to compute surface emissivity at 32um
     50=> open a ticket
     51
     52Joseph:
     53- work on the present day water cycle: strong impact on the physics time step
     54  (as found by Margaux) which makes the water cycle drier. Some retuning needed
     55  frost albedo, contact parameter, variance of the distribution (won't play with that one)
     56- new vdifc for Margaux to test.
     57
     58Siteng:
     59- started with the GCM on Ciclad.
     60
     61Antoine:
     62- mountain slope flows parametrization => only the biggest mountains are now used (6)
     63  also did a test run with 19 biggest mountains (converges to similar results)
     64  still not very good in terms of detached layers at the beginning of the year...
     65- NB: for computations of DSO there is some latitude on choice of underlying factors
     66  for comparisons with MCS
     67- run more years to check convergence.
     68
     69Lucas:
     70- Insight surface pressure measurement drift. Add a correction for sensor temperature
     71  and then 1st and 2nd years match
     72- some divergence with the model around Ls=300-360 to further investigate
     73- also looks at MSL pressure data over 4-5 Mars years
     74- checks the VL data and its interpolated derivation that is used to rescale the MCD
     75
     76Thomas:
     77- MCD slope winds parametrization: putting it all together for all times of day
     78  and location. Still some problems in the night.
     79}}}
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