| | 2 | |
| | 3 | '''10^th^ February 2022''' |
| | 4 | {{{ |
| | 5 | Duration: 50mn |
| | 6 | |
| | 7 | Participants: Ehouarn, Jean-Yves, Thomas, Lucas, Margaux, Jiandong, Christophe, Aymeric, Antoine |
| | 8 | |
| | 9 | News: |
| | 10 | - None |
| | 11 | |
| | 12 | Recent commits: https://trac.lmd.jussieu.fr/Planeto/log |
| | 13 | ============== |
| | 14 | - None |
| | 15 | |
| | 16 | Recent tickets: https://trac.lmd.jussieu.fr/Planeto/report/1 |
| | 17 | ============== |
| | 18 | - None |
| | 19 | |
| | 20 | Hot 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 | |
| | 50 | Jean-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 | |
| | 55 | Thomas: |
| | 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 | {{{ |
| | 64 | Duration: 1h |
| | 65 | |
| | 66 | Participants: Ehouarn, Francois, Christophe, Antoine, Lucas, Thomas, Aymeric |
| | 67 | |
| | 68 | News: |
| | 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 | |
| | 72 | Recent commits: https://trac.lmd.jussieu.fr/Planeto/log |
| | 73 | ============== |
| | 74 | - None |
| | 75 | |
| | 76 | Recent tickets: https://trac.lmd.jussieu.fr/Planeto/report/1 |
| | 77 | ============== |
| | 78 | - None |
| | 79 | |
| | 80 | Hot 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 | |
| | 94 | Thomas: |
| | 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 | {{{ |
| | 103 | Bonjour, |
| | 104 | |
| | 105 | Ehouarn 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 | |
| | 109 | Duration: 80 mn |
| | 110 | |
| | 111 | Participants: Lucas, Siteng, Romain, Christophe, Margaux, Thomas |
| | 112 | Aymeric, Sandrine, Francois, Antony, Jiandong |
| | 113 | |
| | 114 | News: |
| | 115 | - Sandrine's TIRVIM paper is accepted, Siteng's TIRVIM paper is in |
| | 116 | revision |
| | 117 | - Mars Atmosphere Workshop back in preparation.. |
| | 118 | |
| | 119 | Recent commits: https://trac.lmd.jussieu.fr/Planeto/log |
| | 120 | ============== |
| | 121 | Nothing new. |
| | 122 | |
| | 123 | Recent 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 | |
| | 129 | Various 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: |
| | 139 | Problem 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 | }}} |