Changes between Version 3 and Version 4 of Arx2022


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Timestamp:
Feb 10, 2022, 2:12:34 PM (3 years ago)
Author:
cmathe
Comment:

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  • Arx2022

    v3 v4  
    11[ArchiveReport Back] [wiki:Arx2021 Previous Year] [wiki:Arx2023 Next Year]
     2
     3'''10^th^ February 2022'''
     4{{{
     5Duration: 50mn
     6
     7Participants: Ehouarn, Jean-Yves, Thomas, Lucas, Margaux, Jiandong, Christophe, Aymeric, Antoine
     8
     9News:
     10- None
     11
     12Recent commits: https://trac.lmd.jussieu.fr/Planeto/log
     13==============
     14- None
     15
     16Recent tickets: https://trac.lmd.jussieu.fr/Planeto/report/1
     17==============
     18- None
     19
     20Hot topics:
     21==========
     22
     23* Finalizing the DARI request for computing hours (deadline next Monday morning!):
     24- For Mars: Goal: Finalizing GCM6 + producing MCD6
     25  - CO2+water+dust cyle tuning (Antoine)
     26  - non-oro GW (+possible orographic GW re-tuning) Jiandong
     27  - CO2 clouds (Christophe => Lola + Anni) => 50kh ?
     28  - GCM6 runs for MCD6 + validation (Ehouarn, Romain, Thomas) => 50kh?
     29  - Dynamico + OpenMP work (Romain)
     30  - other things?
     31- For Paleo-Mars (past and ancient Mars): => PEM (Romain) + Lucas + Antony => ~400kh
     32  - the work about adding sub-grid slopes (Lucas) can be included in this section
     33
     34* Improving the water and dust cycles (Antoine)
     35- Ran simulations and checked that the non-conservation of water is ~0.2% per year
     36  which is "reasonable" to proceed...
     37- running with different albedos and thermal inertia (800 and 1500) of H2O ice deposit
     38  gets a too dry water cycle in both cases. Now testing with lower albedos for ground ice and frost.
     39- should commit the changes for dust cycle v6 to the trunk
     40- wondering about making a "climatology" from MCS data over MYs to compare to the "clim" simulation
     41
     42* Non-orographic GW (Jiandong)
     43- gets some polar warming which is closer to MCS obs
     44- amplitude of the phase is improved but not perfect.
     45- temperature field not affected below ~40km but winds are.
     46
     47* OpenMP:(Romain)
     48- TBC
     49
     50Jean-Yves:
     51- made comparisons of Deuterium density between GCM MY33 and MAVEN/IUS
     52  D is overall underestimated by the GCM => due to missing ionospheric reactions for D ?
     53  will discuss this with Francisco.
     54
     55Thomas:
     56- the MCD web interface: is adding altitude of observer to spherical projections
     57- working on slope wind model with simple model equation for theta
     58}}}
     59
     60
     61
     62'''3^rd^ February 2022'''
     63{{{
     64Duration: 1h
     65
     66Participants: Ehouarn, Francois, Christophe, Antoine, Lucas, Thomas, Aymeric
     67
     68News:
     69- ACS SWT#13 yesterday and today (resumes at 1pm with Roland talking about Data Assimilation of TIRVIM,
     70  so let's keep this POULDP short!)
     71
     72Recent commits: https://trac.lmd.jussieu.fr/Planeto/log
     73==============
     74- None
     75
     76Recent tickets: https://trac.lmd.jussieu.fr/Planeto/report/1
     77==============
     78- None
     79
     80Hot topics:
     81==========
     82
     83* Improving the water and dust cycles (Antoine)
     84- tests water conservation over 10 sols; non-conservation is from the dynamics mostly
     85  looked at total atmospheric mass evolution, not conserved in dynamics, even without CO2 condensation
     86- tests renormalizing atmospheric mass/water at the beginning of the physics ongoing
     87
     88* Non-orographic GW (Jiandong)
     89- TBC
     90
     91* OpenMP:(Romain)
     92- TBC
     93
     94Thomas:
     95- Slope winds in the MCD: changing the vertical distribution to be more uneven near the surface
     96  improves things.
     97- Some discussion about underlying hypothesis for evaluation of theta lower (surface) boundary condition.
     98}}}
     99
     100
     101'''27^th^ January 2022'''
     102{{{
     103Bonjour,
     104
     105Ehouarn mentionned to me that he had not received last week Mars POULDP minutes... I was initially surprised but after checking, I realise that I only sent them to myself. No wonder ! Oh well. At last here are last weeks minutes :
     106
     107*****************************************
     108
     109Duration: 80 mn
     110
     111Participants: Lucas, Siteng, Romain, Christophe, Margaux, Thomas
     112  Aymeric, Sandrine, Francois, Antony, Jiandong
     113
     114News:
     115- Sandrine's TIRVIM paper is accepted, Siteng's TIRVIM paper is in
     116  revision
     117- Mars Atmosphere Workshop back in preparation..
     118
     119Recent commits: https://trac.lmd.jussieu.fr/Planeto/log
     120==============
     121Nothing new.
     122
     123Recent tickets: https://trac.lmd.jussieu.fr/Planeto/report/1
     124==============
     125- ticket about 32um emissivity: Christophe did add more information
     126- ticket about initracer : christophe updated the ticket
     127
     128
     129Various topics:
     130==============
     131
     132* Thomas : designed a program to obtain the best parameters for his slope winds model. Show test results in various craters.
     133
     134- Problem with the comparison in Korolev because the topography is different in the MCD and in the mesoscale simulations used => Discussion : Aymeric realises that he made this simulation assuming a topography without ice glaciers during studies with Jack Holt...
     135
     136- Discussion : more levels could be used near the surface to optimize the wind calculations at 1 m.
     137
     138* Romain:
     139Problem with crashes of the GCM at the very beggining of test runs after retarting the planetary evolution model.
     140
     141* Siteng Compare TIRVIM near-equatorial semidiurnal tide phase with GCM: when the observation sampling is taken into account, there is a difference up to 3 hours... The semidiurnal wavelength is also affected.
     142
     143* Christophe works on his papers. He has found a little bug in its simulation. Christophe is hoping to join Constantino Listowski's team at CEA (confirmation in one month). Would start on april 1st or may 1st.
     144
     145* Lucas :
     146   - Work on the Planetary Evolution Model with Romain
     147   - Work on water ice on slopes ("Debugging")
     148
     149* Jiandong :
     150   - Tunes the Non-Oro Gravity Wave model to match temperatures.
     151     Progresses are made
     152
     153* Antony
     154   - Dynamico : We should meet and work on validation projects and science
     155     projects with Dynamico => discussion this afternoon : let's wait for
     156     the Mars GCM version 6
     157
     158* Francois
     159   - Finishing the Insight paper as always.
     160   - Will advertise two post-doc positions for the Mars Through Time
     161     Project
     162}}}
    2163
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