Mars-solar wind interaction: LatHyS, an improved parallel 3-D multispecies hybrid model

Ronan Modolo; Sebastien Hess; Marco Mancini; François Leblanc; Jean-Yves Chaufray; David Brain; Ludivine Leclercq; Rosa Esteban Hernandez; Gérard Chanteur; Philippe Weill; Francisco González-Galindo; François Forget; Manabu Yagi; Christian Mazelle

Mars-solar wind interaction: LatHyS, an improved parallel 3-D multispecies hybrid model

Ronan Modolo ¹ Sebastien Hess ^{2, 1} Marco Mancini ^{1, 3} François Leblanc ¹ Jean-Yves Chaufray ¹ David Brain ⁴ Ludivine Leclercq ¹ Rosa Esteban Hernandez ¹ Gérard Chanteur ⁵ Philippe Weill ⁶ Francisco González-Galindo ^{7, 8} François Forget ⁸ Manabu Yagi ^{9, 1} Christian Mazelle ¹⁰

1 HEPPI - LATMOS

LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales

2 ONERA - The French Aerospace Lab [Toulouse]

3 LUTH - Laboratoire Univers et Théories

4 LASP - Laboratory for Atmospheric and Space Physics [Boulder]

5 LPP - Laboratoire de Physique des Plasmas

6 LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales

7 IAA - Instituto de Astrofísica de Andalucía

8 LMD - Laboratoire de Météorologie Dynamique (UMR 8539)

9 Tohoku University [Sendai]

10 IRAP - Institut de recherche en astrophysique et planétologie

Abstract : In order to better represent Mars-Solar wind interaction, we present an unprecedented model achieving spatial resolution down to 50 km, a so far unexplored resolution for global kinetic models of the Martian ionized environment. Such resolution approaches the ionospheric plasma scale height. In practice, the model is derived from a first version described in Modolo et al. [2005]. An important effort of parallelization has been conducted and is presented here. A better description of the ionosphere was also implemented including ionospheric chemistry, electrical conductivities and a drag force modelling the ion-neutral collisions in the ionosphere. This new version of the code, named LatHyS (Latmos Hybrid Simulation), is here used to characterize the impact of various spatial resolutions on simulation results. In addition, and following a global model challenge effort [Brain et al., 2010], we present the results of simulation run for three cases which allows addressing the effect of the supra-thermal corona and of the solar EUV activity on the magnetospheric plasma boundaries and on the global escape. Simulation results showed that global patterns are relatively similar for the different spatial resolution runs but finest grid runs provide a better representation of the ionosphere and display more details of the planetary plasma dynamic. Simulation results suggest that a significant fraction of escaping O+ ions is originated from below 1200 km altitude.

Keywords : Mars Simulation magnetosphere plasma interaction

Document type :

Journal articles

Domain :

Sciences of the Universe [physics] / Astrophysics [astro-ph] / Solar and Stellar Astrophysics [astro-ph.SR]

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