What can be learned from the absence of auroral X-ray emission from Saturn?

To understand the origin and magnitude of the present upper limit observations of Saturn's auroral X‐ray emission, we use simple models based on the mechanism that leads to analogous emission at Jupiter, charge transfer between ion precipitation and atmospheric gas. Several putative sources and...

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Veröffentlicht in:Journal of Geophysical Research 2010, Vol.115 (A10), p.n/a
Hauptverfasser: Hui, Yawei, Cravens, Thomas E., Ozak, Nataly, Schultz, David R.
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Sprache:eng
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