Decametric radiation from Jupiter. I - Morphology of S-burst storms

Details Decametric radiation from Jupiter. I - Morphology of S-burst storms Decametric radiation from Jupiter. I - Morphology of S-burst storms

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..19..296r&link_type=abstract

(Astronomicheskii Vestnik, vol. 19, Oct.-Dec. 1985, p. 296-318) Solar System Research (ISSN 0038-0946), vol. 19, no. 4, April 19

Astronomy and Astrophysics

Astronomy

1

Decametric Waves, Io, Jupiter (Planet), Noise Storms, Planetary Radiation, Radio Bursts, Drift Rate, Radio Spectra, Radio Telescopes, Satellite Orbits, Spectrum Analysis

Scientific paper

Results are reported from monitoring the spectra of S-burst storms on Jupiter in the frequency bands 10-23 MHz over the period 1980-1982. The east-west arm of the UTR-2 broadband decametric telescope was employed for the observations, which covered entire storm durations. S-storms were observed at every location in the Jovian central meridian longitude and Io phase angles outside of 120-200 deg. The storms all group frequency drifts from 60-600 kHz/min, with the drifts being positive near the first Io phase and negative during the second Io phase. The conical radiation patterns are concluded to have frequency-dependent angular structures, with the outer surface of the cone radiating low-frequency emissions and the S-burst frequency originating in the interior of the cone.

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