Polarisation structure of Jupiter's decametre radio bursts

Details Polarisation structure of Jupiter's decametre radio bursts Polarisation structure of Jupiter's decametre radio bursts

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.255..210r&link_type=abstract

Nature, vol. 255, May 15, 1975, p. 210, 211.

Physics

4

Decametric Waves, Jupiter (Planet), Planetary Radiation, Polarization Characteristics, Radio Bursts, Emission Spectra, Histograms, Polarized Electromagnetic Radiation, Radio Spectra

Scientific paper

Sample high-resolution spectra of Jupiter's decameter radio bursts are analyzed in terms of their modulation lanes, or repeated diagonal ridges. The slope of these diagonals, which may be positive or negative, is a function of the System III central meridian longitude of Jupiter. It is concluded that polarization diversity does not occur as a rule in the spectra of modulation lanes.

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