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|a 10.1029/2021GL096990
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|a eng
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|a Wu, S Y
|e verfasserin
|4 aut
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|a Reflection and Refraction of the L-O Mode 5 kHz Saturn Narrowband Emission by the Magnetosheath
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|c 2022
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|a Text
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|a ƒaComputermedien
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|a ƒa Online-Ressource
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|a Date Revised 31.07.2022
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|a published: Print-Electronic
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|a Citation Status PubMed-not-MEDLINE
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|a © 2022. The Authors.
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|a 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 of low plasma density but disappeared in regions of high plasma density. In three cases, NB disappeared immediately after the crossings of Saturn's magnetopause. A possible reflected NB event observed near the magnetosheath is discussed. This mechanism can help explain the 5 kHz NB observed at low latitudes outside the Enceladus plasma torus and their upper frequency limit variations. This mechanism significantly improves the current understanding of the 5 kHz NB
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|a Journal Article
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|a Ye, S Y
|e verfasserin
|4 aut
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|a Fischer, G
|e verfasserin
|4 aut
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|a Jackman, C M
|e verfasserin
|4 aut
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| 700 |
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|a Wang, J
|e verfasserin
|4 aut
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|a Menietti, J D
|e verfasserin
|4 aut
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|a Cecconi, B
|e verfasserin
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|a Long, M Y
|e verfasserin
|4 aut
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|i Enthalten in
|t Geophysical research letters
|d 1984
|g 49(2022), 5 vom: 16. März, Seite e2021GL096990
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|x 0094-8276
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|g volume:49
|g year:2022
|g number:5
|g day:16
|g month:03
|g pages:e2021GL096990
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|u http://dx.doi.org/10.1029/2021GL096990
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