Evidence of Hot Hydrogen in the Exosphere of Mars - INSU - Institut national des sciences de l'Univers Accéder directement au contenu
Communication Dans Un Congrès Année : 2019

Evidence of Hot Hydrogen in the Exosphere of Mars

Résumé

This work is to study the energetic hydrogen atoms present in the exosphere of Mars. Usually this population is not discernible from the thermal H population on account of the large scale height of Mars' atmosphere. However, recent observations under certain conditions with the Hubble Space Telescope reveal the signature of the existence of such a population in the exosphere of Mars. The goal of this study is to understand an characterize the properties of this population and determine its effects on the escape of water from Mars.
Fichier principal
Vignette du fichier
EPSC-DPS2019-960-1.pdf (174.93 Ko) Télécharger le fichier
Origine : Fichiers produits par l'(les) auteur(s)

Dates et versions

insu-04412175 , version 1 (23-01-2024)

Identifiants

Citer

Dolon Bhattacharyya, John Clarke, Majd Mayyasi, Jean-Yves Chaufray, Carl Schmidt, et al.. Evidence of Hot Hydrogen in the Exosphere of Mars. EPSC-DPS Joint Meeting 2019,, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-960-1. ⟨insu-04412175⟩
22 Consultations
7 Téléchargements

Partager

Gmail Facebook X LinkedIn More