Modeling and investigative studies of Jovian low frequency emissions

Details Modeling and investigative studies of Jovian low frequency emissions Modeling and investigative studies of Jovian low frequency emissions

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986plas.rept...44m&link_type=abstract

In NASA, Washington Reports of Planetary Astronomy, 1985 p 44-45 (SEE N87-12407 03-89)

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Computer Programs, Low Frequencies, Planetary Radiation, Ray Tracing, Decametric Waves, Electromagnetic Noise, Io, Kilometric Waves, Magnetic Fields, Noise Pollution

Scientific paper

The Voyager data in a newly produced noise-reduced and recalibrated format has been received. New color spectrograms were developed on high resolution color terminals which display this data. The production of these new spectrograms utilizing the new format data is quite important, because it eliminates a serious problem of noise contamination and miscalibration in the old data set. In addition, a new Jovian plasma model was introduced, which includes the Io torus and accounts for 7 ionic species. The new plasma model is important in the ray tracing of hectometric (HOM) and kilometric (KOM) radiation which may be influenced by the Io torus.

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