| 2 | |
| 3 | |
| 4 | '''6^th^ May 2021''' |
| 5 | {{{ |
| 6 | |
| 7 | Duration:1h30mn |
| 8 | |
| 9 | Participants: Ehouarn, Lucas, Margaux, Christophe, Siteng, Romain, Joseph, Antoine, Thomas, Antony, |
| 10 | Francois |
| 11 | |
| 12 | News: |
| 13 | ==== |
| 14 | - Luca downloaded the latest MCS products and will make an updated MY35 dust scenario. |
| 15 | - Ciclad has been updated with very recent versions of gfortran and ifort. |
| 16 | |
| 17 | Recent commits: https://trac.lmd.jussieu.fr/Planeto/log |
| 18 | ============== |
| 19 | - r2509: scripts to sync git&svn repositories |
| 20 | - r2510: fix example run_month1 script for Ciclad |
| 21 | - r2511: follow-up of r2507 which broke physics/dynamics separation |
| 22 | - r2512: adding "cap_albedo" flag (default .false.) |
| 23 | - r2513: streamfunction utility, look for cu,cv in start.nc => NB by Francois: it could be |
| 24 | coded/computed based on lon/lat coordinate values. Ticket? |
| 25 | - r2514: update of r2507 to write the correct ztime in restartfi.nc files (dynamico case) |
| 26 | avoid writing diagfi with dynamico + XIOS calendar |
| 27 | - r2515: vdifc update. (latent heat of sublimation + implicit scheme + |
| 28 | adaptative sub-timestep + handling hdo as well) |
| 29 | |
| 30 | Recent tickets: https://trac.lmd.jussieu.fr/Planeto/report/1 |
| 31 | ============== |
| 32 | - #76: make a utility to compute 32-um surface emissivity to compare to MCS data |
| 33 | |
| 34 | Ongoing discussions: |
| 35 | =================== |
| 36 | |
| 37 | * Brutal drying up in the thermosphere issue: (Francisco, Margaux, Francois) |
| 38 | From Francois's checks, lowering the threshold in watercloud_mod to 1.e-16 is OK. |
| 39 | It should not be a hard coded number...e.g. real,parameter :: qpere_min = 1.e-16 which |
| 40 | is in traceur_mod.F |
| 41 | Margaux ran some simulations and confirms 1.e-16 works well. => Margaux will commit the update |
| 42 | |
| 43 | * Crash with unexpected unrealistic HDO ratio: (Jean-Yves, Margaux, Ehouarn) |
| 44 | HDO_ice ratio of 4000 from the dynamics |
| 45 | Problem identified (with isotopes) to comes from the dynamics. |
| 46 | To be continued... |
| 47 | |
| 48 | * Dynamico-Mars: |
| 49 | - XIOS output calendar: To keep it "clean" we tell it a timestep is 1s and that the |
| 50 | number of physics time steps is the length of the day. And impose an output time axis |
| 51 | labelled in days and fraction thereof. |
| 52 | - Loading tracers from start file now OK; requires reading a (new generation) tracer.def file |
| 53 | |
| 54 | Lucas: |
| 55 | - MSL/REM pressure data & Insight surface pressure investigations |
| 56 | will compare with GCM runs provided by Francois |
| 57 | |
| 58 | Francois: |
| 59 | - compiled outputs from various simulations for Lucas. |
| 60 | - updated zrecast sent to Ehouarn & Christophe |
| 61 | |
| 62 | Siteng: |
| 63 | - ran GCM for MY35, comparing with TIRVIM temperatures, larger diurnal variations in the GCM |
| 64 | compared to TIRVIM. runs with iphysiq=10; will test with iphysiq=5 |
| 65 | |
| 66 | Antoine: |
| 67 | - topflow runs. Ran a second year; seems quite converged wrt first year. |
| 68 | - MCS-GCM ratio when comparing DSO: does the extrapolation/column recomputation of |
| 69 | GCM outputs to test versus MCS product to find if their is a constant ratio, |
| 70 | but there doesn't seem to be... |
| 71 | |
| 72 | Romain: |
| 73 | - is putting tab_control in XIOS outputs |
| 74 | - will now test Dynamico with tracers (i.e CO2, water, dust cycles included) |
| 75 | - PEM (Planetary Evolution Model) reads/writes start files. |
| 76 | |
| 77 | Joseph: |
| 78 | - present day water cycle tuning: work in progress. |
| 79 | - testing taking a water contact parameter temperature dependence into account |
| 80 | }}} |