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- W530414 abstract "Titan presents a dense atmosphere, which is ionised by solar EUV radiation and particle ionisation, e.g. impacting electrons and ions from the co-rotating magnetosphere of Saturn. In addition, ion transport from dayside to nightside is believed to play a role in the formation of the ionosphere. Until now Cassini has performed close to 70 flybys of Titan, showing that the ionosphere of the moon exhibits a highly complex structure that varies with external conditions, such as solar illumination and variations in Saturn’s magnetosphere." @default.
- W530414 created "2016-06-24" @default.
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- W530414 date "2010-05-01" @default.
- W530414 modified "2023-09-28" @default.
- W530414 title "Observations of ionospheric currents at Titan" @default.
- W530414 hasPublicationYear "2010" @default.
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