Non-Io decametric radiation from Jupiter at frequencies above 30 MHz

Details Non-Io decametric radiation from Jupiter at frequencies above 30 MHz Non-Io decametric radiation from Jupiter at frequencies above 30 MHz

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....86..339b&link_type=abstract

Astronomy and Astrophysics, vol. 86, no. 3, June 1980, p. 339-341.

Astronomy and Astrophysics

Astrophysics

7

Decametric Waves, Jupiter (Planet), Planetary Radiation, Io, Radiant Flux Density, Space Exploration, Jupiter, Radiation, Decameter Waves, Observations, Voyager 1, Data, Emissions, Frequency, Flux, Density, Theoretical Studies, Models, Analysis, Io, Satellites

Scientific paper

Jovian Non-Io decametric radio events extending to frequencies of 30 MHz and above have been found in the Meudon-Nancay observations during 1978 and 1979, in the Voyager 1 PRA observations during February and March, 1979 and in the University of Colorado Radio Astronomy Observatory catalogue for 1960 to 1975. These events, which appear to be mostly associated with the Jovian A-source, query the existence of a cut-off, a little below 30 MHz, for the Non-Io emission and suggest the possibility of a single mechanism for both the Io and the Non-Io radiation.

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