Relation of Jupiter's Radio Emission at Long Wavelengths to Solar Activity
Abstract
Since the spring of 1960 a strong positive correlation between Jupiter's decametric emission and solar decametric continuum emission observed at Boulder has been evident. The time delay of 1 to 2 days, with solar emission preceding Jupiter's emission, suggests that fast solar corpuscles, at velocities of the order of 0.1 c, are directly involved in the planet's atmosphere or magnetic field.
References
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Published In
Science
Volume 132 | Issue 3435
28 October 1960
28 October 1960
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© 1960.
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Published in print: 28 October 1960
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