In ecliptic observations of Jovian radio emissions by ULYSSES - Comparison with Voyager results

Details In ecliptic observations of Jovian radio emissions by ULYSSES - Comparison with Voyager results In ecliptic observations of Jovian radio emissions by ULYSSES - Comparison with Voyager results

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19.1307l&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 19, no. 12, June 19, 1992, p. 1307-1310. Research supported by CNES.

Astronomy and Astrophysics

Astronomy

19

Jupiter (Planet), Planetary Radiation, Plasma Waves, Radio Emission, Ulysses Mission, Voyager Project, Kilometric Waves, Low Frequencies, Radio Astronomy, Solar Radio Emission, Solar Wind

Scientific paper

During the Ulysses inbound cruise to Jupiter the Unified Radio and Plasma Wave (URAP) experiment observed a variety of the planet's radio components in the frequency range below 1 MHz. Most of these emissions were already detected by the Voyager Radio Astronomy and Plasma Wave experiments, however, with much less sensitivity and different spectral coverage. These different radio components within the URAP dynamic spectra are identified, and their appearance with the previous Voyager observations are compared.

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