Evolution of the spectral fine structure of Jupiter's decametric S-storms

Details Evolution of the spectral fine structure of Jupiter's decametric S-storms Evolution of the spectral fine structure of Jupiter's decametric S-storms

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991em%26p...53..157r&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 53, May 1991, p. 157-182.

Physics

Optics

19

Decametric Waves, Evolution (Development), Fine Structure, Jupiter (Planet), Magnetic Storms, Planetary Radiation, Radio Bursts, Acousto-Optics, Io, Radio Spectroscopy

Scientific paper

High-resolution spectra of Jupiter's decametric S-storms are examined with an acoustooptical radio spectrograph operating over the frequency range 20-30 MHz. In 1985-1989 20 S-storms were recorded in the Io-B region, showing only a slight average zoning effect of certain types of fine structure, with sporadic S-bursts occurring most frequently in the early CML values, and S-trains in the late values. There is no precise storm-to-storm correspondence, nor any Io-B centered zones in which the various types of fine structure can be accurately placed.

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