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Low order effect of crand input in the Jovian atmosphere
Authors:Martin S Spergel
Institution:(1) York College of the City University of New York, N.Y., Jamaica, USA
Abstract:Modeling of the Jovian atmosphere shows that cosmic ray induced albedo neutron decay is inadequate to account for Pioneer 10 and 11 projected electron levels on Jupiter. High energy solar protons must also be excluded as an important neutron decay source. Analysis of neutron flux data near the top of the Jovian atmosphere can lead to the determination of He/H2 and3He/4He ratios for the Jovian atmosphere.
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