Maximum frequency of the decametric radiation from Jupiter

Details Maximum frequency of the decametric radiation from Jupiter Maximum frequency of the decametric radiation from Jupiter

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....90l...4b&link_type=abstract

Astronomy and Astrophysics, vol. 90, no. 1-2, Oct. 1980, p.L4-L6. Research supported by the Centre National de la Recherche Sci

Astronomy and Astrophysics

Astronomy

5

Decametric Waves, Jupiter (Planet), Planetary Radiation, Radio Emission, Gyrofrequency, Io, Spaceborne Astronomy, Jupiter, Radiation, Decameter Waves, Wavelengths, Data, Frequency, Observations, Emissions, Comparisons, Satellites, Io, Voyager, Earth-Based Observations, Source Medium

Scientific paper

The upper frequency limits of Jupiter's decametric radio emission are found to be essentially the same when observed from the earth or, with considerably higher sensitivity, from the Voyager spacecraft close to Jupiter. This suggests that the maximum frequency is a real cut-off corresponding to a maximum gyrofrequency of about 38-40 MHz at Jupiter. It no longer appears to be necessary to specify different cut-off frequencies for the Io and non-Io emission as the maximum frequencies are roughly the same in each case.

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