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Short periodicities in low-frequency plasma waves at Saturn
Journal article   Open access   Peer reviewed

Short periodicities in low-frequency plasma waves at Saturn

J. F. Carbary, W. S. Kurth and D. G. Mitchell
Journal of geophysical research. Space physics, Vol.121(7), pp.6562-6572
07/01/2016
DOI: 10.1002/2016JA022732
url
https://doi.org/10.1002/2016JA022732View
Published (Version of record) Open Access

Abstract

Short-period amplitude modulations (similar to 60min period) have been detected in the similar to 100Hz plasma wave emissions observed by the Radio Plasma Wave Science instrument on the Cassini spacecraft in orbit around Saturn. These periodicities were detected throughout the mission from mid-2004 to the present, and this is the first statistical study of them. The modulations are observed throughout the magnetosphere and can last from similar to 2h to similar to 20h, although the duration may be biased by spacecraft observing conditions. The periodicities are statistically much more likely to be seen at high latitudes, both north and south, and at local times between dusk and midnight. When corrected for latitude and local time, the occurrence frequency has declined in time since 2005. Considering all observations, the mean period of these events is 65.320.7min, with a peak (modal value) at 63.3min. The period has no dependence on local time or latitude. Alfven waves have interhemispheric transit times commensurate with the mean periods and should thus be considered principal candidates for their production.
Astronomy & Astrophysics Physical Sciences Science & Technology

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