ULYSSES observations of escaping VLF emissions from Jupiter

Details ULYSSES observations of escaping VLF emissions from Jupiter ULYSSES observations of escaping VLF emissions from Jupiter

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19..649k&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 19, April 3, 1992, p. 649-652.

Physics

21

Jupiter (Planet), Planetary Radiation, Radio Emission, Ulysses Mission, Very Low Frequencies, Hydrodynamic Ram Effect, Solar Wind, Type 3 Bursts

Scientific paper

The Ulysses URAP experiment has detected Jovian radio emissions in the VLF range at distances from Jupiter in excess of 1.5 AU. The URAP observations represent the first synoptic observations of Jupiter in the VLF band, from 3 to 30 kHz. In this band lie the low-frequency extent of the bKOM emission, the escaping continuum emission, and the Jovian type IIIs. Initial results indicate that the continuum varies in frequency with the solar wind ram pressure at Jupiter, whereas, the Jovian type IIIs appear to be controlled to some extent by the planetary rotation, often appearing when system III longitude 100 deg faces the spacecraft.

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