Zobrazeno 1 - 10
of 106
pro vyhledávání: '"E. Millour"'
Autor:
L. Lange, F. Forget, M. Vincendon, A. Spiga, E. Vos, O. Aharonson, E. Millour, A. Bierjon, R. Vandemeulebrouck
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 21, Pp n/a-n/a (2023)
Abstract Massive reservoirs of subsurface water ice in equilibrium with atmospheric water vapor are found poleward of 45° latitude on Mars. The absence of CO2 frost on steep pole‐facing slopes and simulations of atmospheric‐soil water exchanges
Externí odkaz:
https://doaj.org/article/622cf02a8e7e49a9913c80acd86405cb
Autor:
M. Golombek, N. H. Warner, J. A. Grant, E. Hauber, V. Ansan, C. M. Weitz, N. Williams, C. Charalambous, S. A. Wilson, A. DeMott, M. Kopp, H. Lethcoe-Wilson, L. Berger, R. Hausmann, E. Marteau, C. Vrettos, A. Trussell, W. Folkner, S. Le Maistre, N. Mueller, M. Grott, T. Spohn, S. Piqueux, E. Millour, F. Forget, I. Daubar, N. Murdoch, P. Lognonné, C. Perrin, S. Rodriguez, W. T. Pike, T. Parker, J. Maki, H. Abarca, R. Deen, J. Hall, P. Andres, N. Ruoff, F. Calef, S. Smrekar, M. M. Baker, M. Banks, A. Spiga, D. Banfield, J. Garvin, C. E. Newman, W. B. Banerdt
Publikováno v:
Nature Communications, Vol 11, Iss 1, Pp 1-11 (2020)
The InSight spacecraft landed on Mars on November 2018. Here, the authors characterize the surficial geology of the landing site and compare with observations and models derived from remote sensing data prior to landing and from ongoing in situ geoph
Externí odkaz:
https://doaj.org/article/4ddb238f4e9a41b193efa61d62e46113
Autor:
S. Erard, B. Cecconi, P. Le Sidaner, C. Chauvin, A. P. Rossi, M. Minin, T. Capria, S. Ivanovski, B. Schmitt, V. Génot, N. André, C. Marmo, A. C. Vandaele, L. Trompet, M. Scherf, R. Hueso, A. Määttänen, B. Carry, N. Achilleos, J. Soucek, D. Pisa, K. Benson, P. Fernique, E. Millour
Publikováno v:
Data Science Journal, Vol 19, Iss 1 (2020)
The Europlanet-2020 programme, which ended on Aug 31st, 2019, included an activity called VESPA (Virtual European Solar and Planetary Access), which focused on adapting Virtual Observatory (VO) techniques to handle Planetary Science data. This paper
Externí odkaz:
https://doaj.org/article/9f48d0beb48d437782d2dfebf61b009b
Autor:
K. S. Olsen, A. A. Fedorova, A. Trokhimovskiy, F. Montmessin, F. Lefèvre, O. Korablev, L. Baggio, F. Forget, E. Millour, A. Bierjon, J. Alday, C. F. Wilson, P. G. J. Irwin, D. A. Belyaev, A. Patrakeev, A. Shakun
Publikováno v:
Journal of Geophysical Research: Planets. 127
The mid-infrared channel of the Atmospheric Chemistry Suite (ACS MIR) onboard the ExoMars Trace Gas Orbiter is capable of observing the infrared absorption of ozone (O3) in the atmosphere of Mars. During solar occulations, the 003←000 band (3000-30
Autor:
P. Vlasov, N. Ignatiev, S. Guerlet, D. Grassi, O. Korablev, А. Grigoriev, A. Shakun, D. Patsaev, I. Maslov, L. Zasova, M. Luginin, A. Trokhimovskiy, E. Millour, F. Forget, R. Haus, G. Arnold, F. Montmessin
Publikováno v:
Journal of Geophysical Research: Planets. 127
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
S. Guerlet, N. Ignatiev, F. Forget, T. Fouchet, P. Vlasov, G. Bergeron, R. M. B. Young, E. Millour, S. Fan, H. Tran, A. Shakun, A. Grigoriev, A. Trokhimovskiy, F. Montmessin, O. Korablev
Publikováno v:
Journal of Geophysical Research: Planets. 127
The Atmospheric Chemistry Suite (ACS) onboard the ExoMars Trace Gas Orbiter (TGO) monitors the Martian atmosphere through different spectral intervals in the infrared light. We present a retrieval algorithm tailored to the analysis of spectra acquire
Autor:
E. Vos, O. Aharonson, N. Schörghofer, F. Forget, E. Millour, L. Rossi, M. Vals, F. Montmessin
Exposed scarps images and ice-penetrating radar measurements in the North Polar Layered Deposits (NPLD) of Mars show alternating layers that provide an archive of past climate oscillations, that are thought to be linked to orbital variations, akin to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5990bd7a55b9bc73026bb227f1c12a7d
Autor:
A. Määttänen, C. Mathé, J. Audouard, C. Listowski, E. Millour, F. Forget, F. González-Galindo, L. Falletti, D. Bardet, L. Teinturier, M. Vals, A. Spiga, F. Montmessin
Publikováno v:
Icarus. 385:115098
We have implemented full CO ice cloud microphysics into the LMD Mars Global Climate Model (MGCM) and we have conducted the first global simulations. The microphysical model implementation follows the modal scheme used for water ice cloud microphysics