Radio emission detected from Io - Evidence for radiation belts

Details Radio emission detected from Io - Evidence for radiation belts Radio emission detected from Io - Evidence for radiation belts

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..622m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Nov. 1979, p. 622-624.) Soviet Astronomy Letters, vol. 5, Nov.-Dec. 1979, p. 333, 33

Astronomy and Astrophysics

Astronomy

Io, Planetary Radiation, Radiation Belts, Radio Emission, Brightness Temperature, Centimeter Waves, Decametric Waves, Planetary Magnetic Fields, Satellite Atmospheres

Scientific paper

Radio emission from the Jovian satellite Io has been recorded by the RATAN-600 radio telescope at wavelengths of 2.08 and 3.9 cm. Io's brightness temperature at the two wavelengths is 190 and 600 K. Apparently Io possesses significant radiation belts, and thereby a magnetic field. The decameter bursts of Jupiter might be attributable to processes in the magnetosphere of Io.

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