The Jovian S-bursts. I - Occurrence with L-bursts and frequency limit

Details The Jovian S-bursts. I - Occurrence with L-bursts and frequency limit The Jovian S-bursts. I - Occurrence with L-bursts and frequency limit

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....86..342l&link_type=abstract

Astronomy and Astrophysics, vol. 86, no. 3, June 1980, p. 342-348.

Astronomy and Astrophysics

Astronomy

13

Decametric Waves, Jupiter (Planet), Planetary Radiation, Radio Astronomy, Radio Bursts, Superhigh Frequencies, Ultrahigh Frequencies, Antenna Arrays, Io, Microwave Antennas, Microwave Emission, Jupiter, Radio Emissions, Bursts, Spectrum, Frequency, Regions, Io, Satellites, Equipment, Observations, Data, Storms, Polarization, Diagrams, Bandwidths, Brightness Temperature

Scientific paper

The first spectra of Jovian radio emission in which S bursts can be observed over a wide range of frequencies (20 MHz) during storms lasting two or three hours are examined. It is shown that the S bursts occur only in two regions (Io-controlled emission) of the Io-CML plane with a probability of occurrence reaching 60 percent. The association of the S bursts with the more lasting and broad band L bursts is closely related to the Io-CML configuration, as is the maximum frequency of emission which has not been observed to exceed 33 MHz. Three sections are defined in the Io B-region, in which the S bursts occur alone with a maximum frequency of emission lower than 25 MHz, the S bursts occur superimposed on the L bursts, and the L bursts occur alone.

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