Jovian S-burst observations at 32 MHz

Details Jovian S-burst observations at 32 MHz Jovian S-burst observations at 32 MHz

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.272...38d&link_type=abstract

Nature, vol. 272, Mar. 2, 1978, p. 38-40. NSF-NASA-supported research.

Astronomy and Astrophysics

Astronomy

15

Drift Rate, Jupiter (Planet), Planetary Radiation, Radio Astronomy, Radio Bursts, Superhigh Frequencies, Electron Bunching, Io, Magnetic Effects, Magnetic Flux, Planetary Ionospheres, Spectrographs, Spectrum Analysis, Trapped Particles, Ultrahigh Frequencies, Jupiter, Radioemissions, Io, Radio Waves, Radio Bursts, Bursts

Scientific paper

Drift rates for S-burst emissions from Jupiter are studied. The burst spectra, recorded in the frequency range near 32 MHz, provide a qualitative illustration of the behavior of electron bunches shortly after injection into the Io-associated magnetic flux tube. The morphology of the spectra may be taken as support for the hypothesis of an ionospheric acceleration mechanism influencing the flow of electrons.

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