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

Tsurutani, B.T.; Arballo, J.K.; Ho, C.M.; Lin, N.G.; Kellogg, P.J.; Cornileau-Wehrlin, N.; Krupp, N.

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