Physics
Scientific paper
Jun 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986em%26p...35...93g&link_type=abstract
Earth, Moon, and Planets (ISSN 0167-9295), vol. 35, June 1986, p. 93-115.
Physics
5
Jupiter Atmosphere, Planetary Radiation, Planetology, Space Plasmas, Synchrotron Radiation, Decametric Waves, Electron Bunching, Maser Outputs, Planetary Magnetospheres, Superhigh Frequencies, Ultrahigh Frequencies
Scientific paper
The shadow events in the dynamic spectra of Jovian decametric emission are explained as the result of interaction between electron bunches responsible for S and L emissions. The relevant dispersion relation is derived for the fast extraordinary mode in the cold magnetospheric plasma in the presence of S and L electron bunches. The growth rate of the synchrotron maser instability is studied in the presence and absence of S-electrons. It is shown that the synchrotron maser instability responsible for L-emission can be temporarily quenched by the invasion of S-electrons, thereby stopping the L-emission. The theory accounts for various observed features of the shadow events.
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