The Drivers of the Martian Bow Shock Location: A Statistical Analysis of Mars Atmosphere and Volatile EvolutioN and Mars Express Observations

The Martian interaction with the solar wind leads to the formation of a bow shock upstream of the planet. The shock dynamics appear complex, due to the combined influence of external and internal drivers. The extreme ultraviolet fluxes and magnetosonic Mach number are known major drivers of the shoc...

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Detalles Bibliográficos
Autores principales: Garnier, P., Jacquey, C., Gendre, X., Génot, V., Mazelle, C., Fang, X., Gruesbeck, J. R., Sánchez‐Cano, B., Halekas, J. S.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2022
Materias:
Research Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9287072/
https://www.ncbi.nlm.nih.gov/pubmed/35865127
http://dx.doi.org/10.1029/2021JA030147

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9287072/
https://www.ncbi.nlm.nih.gov/pubmed/35865127
http://dx.doi.org/10.1029/2021JA030147

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