Influence of the solar wind dynamic pressure on the ion precipitation: MAVEN observations and simulation results
Résumé
In this work, we compare simulation of the precipitating flux for different solar wind dynamic pressure with MAVEN observations. In particular, we focus on the fluxes of precipitating ion towards Mars' atmosphere as seen by MAVEN/SWIA (cs product), an energy and angular ion spectrometer [1]. We also use LatHyS, which is a 3D multispecies parallelized hybrid model that describes the formation of Mars electromagnetic environment induced by its interaction with the solar wind [2].
Domaines
Planète et Univers [physics]| Origine | Fichiers produits par l'(les) auteur(s) |
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