Carbon Ion Fluxes at Mars: First Results of Tailward Flows From MAVEN‐STATIC

Characterizing C(+) ions in the Martian ionosphere is important for understanding the history of the Martian atmosphere and surface due to its place in understanding carbon escape. Measuring minor ions, like C(+), which are close in mass to major atmospheric ions, in this case O(+), is difficult, re...

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Detalles Bibliográficos
Autores principales: Pickett, N. B., McFadden, J. P., Fowler, C. M., Hanley, K. G., Benna, M.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2021
Materias:
Research Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9286460/
https://www.ncbi.nlm.nih.gov/pubmed/35865028
http://dx.doi.org/10.1029/2021JA029635

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9286460/
https://www.ncbi.nlm.nih.gov/pubmed/35865028
http://dx.doi.org/10.1029/2021JA029635

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