Oxygen Ion Energization at Mars: Comparison of MAVEN and Mars Express Observations to Global Hybrid Simulation

Author:

Jarvinen R.12ORCID,Brain D. A.3ORCID,Modolo R.4ORCID,Fedorov A.5,Holmström M.6ORCID

Affiliation:

1. Finnish Meteorological Institute; Helsinki Finland

2. Department of Electronics and Nanoengineering, School of Electrical Engineering; Aalto University; Espoo Finland

3. Laboratory for Atmospheric and Space Physics; University of Colorado Boulder; Boulder CO USA

4. LATMOS/IPSL, UVSQ Université Paris-Saclay, UPMC University Paris CNRS; Guyancourt France

5. Université de Toulouse, UPS-OMP, IRAP; Toulouse France

6. Swedish Institute of Space Physics; Kiruna Sweden

Funder

Centre National de la Recherche Scientifique

Centre National d’Etudes Spatiales

Observatoire de Paris

Universite Paul Sabatier

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference48 articles.

1. ASPERA-3 on Mars Express;Barabash;Icarus,2006

2. Martian atmospheric erosion rates;Barabash;Science,2007

3. A strong seasonal dependence in the Martian hydrogen exosphere;Bhattacharyya;Geophysical Research Letters,2015

4. The Zoltan and Isorropia parallel toolkits for combinatorial scientific computing: Partitioning, ordering, and coloring;Boman;Scientific Programming,2012

5. Mars Global Ionosphere-Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere;Bougher;Journal of Geophysical Research: Planets,2015

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