Francois Forget
Centre National D'Etudes Spatiales
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40th International Conference on Environmental Systems | 2010
Aymeric Spiga; Vincent Bourrier; Francois Forget; Ehouarn Millour; L. Montabone; J.-B. Madeleine; L. Solovyeva; M.-C. Desjean; J.-P. Huot; S.R. Lewis; Francisco Gonzalez-Galindo; Miguel Angel Lopez-Valverde; S Portigliotti; M. Dumontel; L. Lorenzoni; T. Blancquaert
In order to allow safe entry descent and landing, as well as mission surface operations, constraints apply to the selection of suitable landing sites. These constraints are defined in terms of general characteristics related to the specific mission profile (interplanetary transfer, waiting orbit injection and orbital waiting period and eclipse mitigation strategies) and to the EDL operations (entry conditions and environment, safe operation of the descent system with parachute deceleration, controlled rockets braking, touchdown with vented airbags). Most constraints are relative to « static » properties such as the geographical location, the altimetry, and the soil thermophysical constants. Few constraints are relative to the « dynamical » properties of the atmosphere, i.e. meteorological variations of density, temperature and winds, notwithstanding these are the most crucial characteristics to predict so as to ensure the success of the EDL phase. Martian mesoscale and microscale meteorological models are one of the relevant tools that can be used to predict the local and regional meteorological variability likely to be encountered at several proposed landing ellipses during Entry, Descent, and Landing. Most of the atmospheric hazards in the Martian lower atmosphere are not evident in current observational data and general circulation model simulations and can only be ascertained through mesoscale modeling of the region. The Laboratoire de Meteorologie Dynamique (LMD) Mesoscale Model is a versatile simulator of the Martian atmosphere and environment at horizontal scales ranging from hundreds of kilometers to tens of meters. Specific simulations with relevancy to assessment of atmospheric hazards possibly encountered in Martian landing sites can be carried out with such a tool. The need for accurate and realistic Martian mesoscale modeling remains critical for the design of upcoming missions to Mars (e.g., Mars Science Laboratory, ExoMars).
European Planetary Science Congress 2015 | 2015
E. Millour; Francois Forget; Aymeric Spiga; T. Navarro; J.-B. Madeleine; L. Montabone; Alizée Pottier; Franck Lefèvre; Franck Montmessin; Jean-Yves Chaufray; Miguel Angel Lopez-Valverde; Francisco Gonzalez-Galindo; Stephen R. Lewis; P. L. Read; J.-P. Huot; M.-C. Desjean
Archive | 2007
J.-B. Madeleine; Francois Forget; James W. Head; B. Levrard; Franck Montmessin
Archive | 2017
Robert M. Haberle; R. Todd Clancy; Francois Forget; Michael D. Smith; Richard W. Zurek
Archive | 2007
J.-B. Madeleine; Francois Forget; James W. Head; B. Levrard; Franck Montmessin
Icarus | 2013
S. M. Clifford; Kenji Yoshikawa; Shane Byrne; William B. Durham; David A. Fisher; Francois Forget; Michael H. Hecht; Peter W. H. Smith; Leslie Kay Tamppari; Timothy N. Titus; Richard W. Zurek
Archive | 2011
J.-B. Madeleine; Francois Forget; Ehouarn Millour
Astronomy and Astrophysics - A&A | 2017
Martin Turbet; Emeline Bolmont; Jérémy Leconte; Francois Forget; Franck Selsis; Gabriel Tobie; Anthony Caldas; Joseph Naar; Michaël Gillon
Archive | 2011
Robin Wordsworth; Francois Forget; Ehouarn Millour; J.-B. Madeleine; Robert M. Haberle; Vincent Eymet
Archive | 2010
R. Todd Clancy; Brad J. Sandor; M. J. Wolff; M. D. Smith; Scott L. Murchie; F. P. Seelos; Armin Kleinböhl; David Michael Kass; Fabrice Lefevre; Francois Forget