Plasma Double Layers at the Boundary Between Venus and the Solar Wind

The solar wind is slowed, deflected, and heated as it encounters Venus's induced magnetosphere. The importance of kinetic plasma processes to these interactions has not been examined in detail, due to a lack of constraining observations. In this study, kinetic‐scale electric field structures ar...

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Detalles Bibliográficos
Autores principales: Malaspina, D. M., Goodrich, K., Livi, R., Halekas, J., McManus, M., Curry, S., Bale, S. D., Bonnell, J. W., de Wit, T. Dudok, Goetz, K., Harvey, P. R., MacDowall, R. J., Pulupa, M., Case, A. W., Kasper, J. C., Korreck, K. E., Larson, D., Stevens, M. L., Whittlesey, P.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2020
Materias:
Research Letters
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7757269/
https://www.ncbi.nlm.nih.gov/pubmed/33380758
http://dx.doi.org/10.1029/2020GL090115

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7757269/
https://www.ncbi.nlm.nih.gov/pubmed/33380758
http://dx.doi.org/10.1029/2020GL090115

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