Reflection and Refraction of the L‐O Mode 5 kHz Saturn Narrowband Emission by the Magnetosheath

The reflection‐by‐sheath mechanism of 5 kHz narrowband emissions (NB) at Saturn is confirmed by Cassini observations during several crossings of the magnetopause, which show that the 5 kHz NB can be prevented from escaping Saturn's magnetosphere. The L‐O mode 5 kHz NB remained visible in areas...

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Detalles Bibliográficos
Autores principales: Wu, S. Y., Ye, S. Y., Fischer, G., Jackman, C. M., Wang, J., Menietti, J. D., Cecconi, B., Long, M. Y.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2022
Materias:
Research Letter
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9285440/
https://www.ncbi.nlm.nih.gov/pubmed/35859935
http://dx.doi.org/10.1029/2021GL096990

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9285440/
https://www.ncbi.nlm.nih.gov/pubmed/35859935
http://dx.doi.org/10.1029/2021GL096990

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