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Detailed Reference Information |
Kaiser, M.L. (1993). Time-variable magnetospheric radio emissions from Jupiter. Journal of Geophysical Research 98: doi: 10.1029/93JE01279. issn: 0148-0227. |
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Jupiter is the source of a large number of independent nonthermal radio sources, all of which vary with time. The known causes of the variations include planetary rotation modulation, modulation by Io and/or its torus, and influence by the solar wind which can reach surprisingly deep into the Jovian magnetosphere. However, a significant number of radio variations, both short-term and long-term, are not currently explained by any known mechanism. |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Radio Science, Radio astronomy, Solar Physics, Astrophysics, and Astronomy, Radio emissions, Magnetospheric Physics, Planetary magnetospheres |
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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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