dc.contributor.author |
Bolton, S.J. |
en_US |
dc.contributor.author |
Thorne, R.M. |
en_US |
dc.date.accessioned |
2004-10-03T03:39:09Z |
|
dc.date.available |
2004-10-03T03:39:09Z |
|
dc.date.issued |
1995 |
en_US |
dc.identifier.citation |
Geophysical Research Letters |
en_US |
dc.identifier.clearanceno |
95-0740 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/30875 |
|
dc.description.abstract |
The impact comet SL-9 with Jupiter induced a number of variations in Jupiter's synchrotron radiation, including an increase in emission intensity, spectral changes, and a possible broadening in the latitudinal distribution of the emission. Considered are three potential mechanisms for inducing such effects (electron acceleration, radial diffusion, and pitch-angle scattering), and their consequences. |
en_US |
dc.format.extent |
231669 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
|
dc.subject.other |
Jupiter Jovian synchrotron variability synchrotron radiation comet SL-9 |
en_US |
dc.title |
Assessment of Mechanisms for Jovian Synchrotron Variability Associated with Comet SL-9 |
en_US |