Relation of Jupiter's Radio Emission at Long Wavelengths to Solar Activity

Details Relation of Jupiter's Radio Emission at Long Wavelengths to Solar Activity Relation of Jupiter's Radio Emission at Long Wavelengths to Solar Activity

Oct 1960

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1960sci...132.1250w&link_type=abstract

Science, Volume 132, Issue 3435, pp. 1250-1252

Physics

15

Scientific paper

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.

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