The Largest Electron Differential Energy Flux Observed at Mars by the Mars Express Spacecraft, 2004–2016

The goal of this paper is to understand the processes by which solar wind electrons are energized in the Martian magnetosphere and how this compares to processes at Venus and Earth. Each is unique in the source of its magnetic field topology and how this influences electron energization. To achieve...

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Detalles Bibliográficos
Autores principales: Frahm, R. A., Winningham, J. D., Coates, A. J., Gérard, J.‐C., Holmström, M., Barabash, S.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2018
Materias:
Research Articles
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6473521/
https://www.ncbi.nlm.nih.gov/pubmed/31032167
http://dx.doi.org/10.1029/2018JA025311

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6473521/
https://www.ncbi.nlm.nih.gov/pubmed/31032167
http://dx.doi.org/10.1029/2018JA025311

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