Probing Jupiter's deep atmosphere and interior structure: a flyby mission proposal
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Engineering topics
Publications and source records attributed to Thorne, R..
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In this paper we discuss recent observations on the study of synchrotron radio emission from Jupiter's inner radiation belts.
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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.
We have constructed a computer model to simulate synchrotron emission from relativistic electrons trapped in Jupiter's magnetic field.
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We applaud the excellent effort and far-reaching results of Newell et al. (1998).