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New Predictions of the Jovian Aurora: Location, Latitudinal Width, and Intensity

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dc.contributor.author Tsurutani, B.T. en_US
dc.contributor.author Arballo, J.K. en_US
dc.contributor.author Ho, C.M. en_US
dc.contributor.author Lin, N.G. en_US
dc.contributor.author Kellogg, P.J. en_US
dc.contributor.author Cornileau-Wehrlin, N. en_US
dc.contributor.author Krupp, N. en_US
dc.date.accessioned 2004-10-03T05:10:21Z
dc.date.available 2004-10-03T05:10:21Z
dc.date.issued 1995-12 en_US
dc.identifier.citation San Francisco, CA en_US
dc.identifier.clearanceno 95-1128 en_US
dc.identifier.uri http://hdl.handle.net/2014/31446
dc.description.abstract A model/theory for the Jovian aurora is formed based on a similar model for the dayside aurora at Earth and recent Ulysses field and particle measurements at Jupiter. Items discussed are plasma boundary layer, wave-particle resonant interactions, and the model's prediction of the aurora's location, latitudinal width, and intensity. en_US
dc.format.extent 51883 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Jupiter Jovian Aurora Ulysses Plasma en_US
dc.title New Predictions of the Jovian Aurora: Location, Latitudinal Width, and Intensity en_US


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