On the fine structure of the Jovian decametric dynamic spectrum

Details On the fine structure of the Jovian decametric dynamic spectrum On the fine structure of the Jovian decametric dynamic spectrum

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994r%26qe...37..445z&link_type=abstract

Radiophysics and Quantum Electronics, Volume 37, Issue 6, pp.445-453

Physics

Scientific paper

A general concept of Jovian decametric radiation is proposed that allows various approaches to the problem of the origin of this radiation to be coordinated. The concept is used to explain the origin of such fine-structure characteristics of the dynamic spectrum as frequency splitting of the high-frequency part of the spectrum and the shape of the spectral arcs. The plasma density and velocity of radiating electrons in the force tube of the planet's magnetic field near the L-shells corresponding to Io.

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