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Divine-garrett model and Jovian synchrotron emission

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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


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