Jovian and terrestrial 'harmonic' radiations

Details Jovian and terrestrial 'harmonic' radiations Jovian and terrestrial 'harmonic' radiations

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977georl...4..121j&link_type=abstract

Geophysical Research Letters, vol. 4, Mar. 1977, p. 121-124.

Physics

5

Harmonic Radiation, Jupiter (Planet), Long Wave Radiation, Planetary Radiation, Earth Magnetosphere, Planetary Magnetic Fields, Planetary Magnetospheres, Solar Wind, Wave Dispersion, Wave Interaction

Scientific paper

It has been proposed by Oya (1974) and Benson (1975) that Jovian decametric radiation (JDR) and terrestrial kilometric radiation (TKR) are produced initially as electrostatic waves which then couple to Z-mode waves close to the upper hybrid resonance. Certain problems concerning an explanation of observations of TKR and JDR on the basis of advanced theories are related to the difference between the dayside and nightside sources of TKR, the beam width of TKR, and the upper cut-off frequency of JDR. A 'harmonic' radiation in the solar wind is considered along with the possibility of a counterpart within the magnetospheres of Jupiter and Earth. An assumption that the magnetic field strength of Saturn is 1 Gauss appears premature.

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