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Detailed Reference Information |
Garrett, H.B., Levin, S.M., Bolton, S.J., Evans, R.W. and Bhattacharya, B. (2005). A revised model of Jupiter's inner electron belts: Updating the Divine radiation model. Geophysical Research Letters 32: doi: 10.1029/2004GL021986. issn: 0094-8276. |
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In 1983, Divine presented a comprehensive model of the Jovian charged particle environment that has long served as a reference for missions to Jupiter. However, in situ observations by Galileo and synchrotron observations from Earth indicate the need to update the model in the inner radiation zone. Specifically, a review of the model for 1 MeV < E < 100 MeV trapped electrons suggests that, based on the new synchrotron observations, the pitch angle distributions within L < 4 need to be updated by introducing two additional components: one near the Jovian magnetic equator and one at high magnetic latitudes. We report modifications to the model that reproduce these observations. The new model improves the fit to synchrotron emission observations and remains consistent with the original fit to the in situ Pioneer and Voyager data. Further modifications incorporating observations from the Galileo and Cassini spacecraft will be reported in the future. |
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Abstract |
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Keywords
Magnetospheric Physics, Energetic particles, trapped, Magnetospheric Physics, Magnetosphere, inner, Magnetospheric Physics, Planetary magnetospheres (5443, 5737, 6033), Planetary Sciences, Solar System Objects, Jupiter, Interplanetary Physics, Energetic particles |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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