Divine-garrett model and Jovian synchrotron emission

Bolton, S.; Levin,  S.; Gulkis,  S.; Klein,  M.; Sault,  R.; Bhattacharya,  B.; Thorne,  R.; Dulk,  G.; Leblanc,  Y.

dc.contributor.author	Bolton, S.	en_US
dc.contributor.author	Levin, S.	en_US
dc.contributor.author	Gulkis, S.	en_US
dc.contributor.author	Klein, M.	en_US
dc.contributor.author	Sault, R.	en_US
dc.contributor.author	Bhattacharya, B.	en_US
dc.contributor.author	Thorne, R.	en_US
dc.contributor.author	Dulk, G.	en_US
dc.contributor.author	Leblanc, Y.	en_US
dc.date.accessioned	2004-09-23T21:08:17Z
dc.date.available	2004-09-23T21:08:17Z
dc.date.issued	2001-03-01	en_US
dc.identifier.citation	Geophysical research letters, v.28, no. 5, pp. 907-910	en_US
dc.identifier.citation	Pasadena, CA, USA	en_US
dc.identifier.clearanceno	00-1581	en_US
dc.identifier.uri	http://hdl.handle.net/2014/15823
dc.description.abstract	Simulations of synchrotron emission from relativistic electrons trapped in Jupiter's magnetic field are used to evaluate the energetic electron distribution of the Divine-Garrett Jupiter radiation belt model at radial distances less than 4 Jovian radii.	en_US
dc.format.extent	165305 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en_US
dc.subject.other	Radial diffusion-models electrons jupiter	en_US
dc.title	Divine-garrett model and Jovian synchrotron emission	en_US