On the origin of the narrow-band splitting at the Jovian decametric cutoff frequency.

Details On the origin of the narrow-band splitting at the Jovian decametric cutoff frequency. On the origin of the narrow-band splitting at the Jovian decametric cutoff frequency.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...305..352s&link_type=abstract

Astronomy and Astrophysics, v.305, p.352

Astronomy and Astrophysics

Astrophysics

4

Planets: Jupiter, Radio Continuum: Solar System, Plasmas, Radiation Mechanisms: Non Thermal

Scientific paper

The origin of the narrow-band splitting in the high-frequency edge of the Jovian decametric emission dynamic spectra is discussed. Three main features were observed on dynamic spectra, giving the possibility to elucidate the problem. A model for the generation of the Jovian decametric radiation is constructed in which plasma and electron cyclotron maser emissions are included. We explain the origin of the splitting and its main features.

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