Analysis of Jovian decametric data: Study of radio emission mechanisms

Details Analysis of Jovian decametric data: Study of radio emission mechanisms Analysis of Jovian decametric data: Study of radio emission mechanisms

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mit..reptq....s&link_type=abstract

Progress Report, 15 Sep. 1982 - 15 Sep. 1984 Massachusetts Inst. of Tech., Cambridge. Research Lab. of Electronics.

Computer Science

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Decametric Waves, Jupiter (Planet), Polarization (Waves), Voyager Project, Algorithms, Computer Graphics, Magnetohydrodynamic Waves, Radio Astronomy, Radio Bursts, Temporal Resolution

Scientific paper

The Voyager 1 and Voyager 2 Planetary Radio Astronomy Experiments (PRA) have produced the finest set of Jovian decametric radio emission data ever obtained. Jovian decametric L-burst and S-burst arcs were characterized and the data reconciled with models for the radio emission geometry and mechanisms. The first major results involve comparisons of the distribution of arc separations with longitudes. The identification and analyses of systematic variations in the PRA data have yielded interesting results, but only the most obvious features of the data were examined. Analyses of the PRA data were extended with the use of new 6-Sec formats that are more sensitive to the S-bursts.

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