Triggered Jovian radio emissions

Details Triggered Jovian radio emissions Triggered Jovian radio emissions

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985georl..12..179c&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 12, April 1985, p. 179-182.

Physics

11

Auroral Zones, Jupiter (Planet), Planetary Radiation, Radio Emission, Solar Radio Bursts, Voyager 1 Spacecraft, Bandwidth, Wavelengths, Jupiter, Radio Emissions, Radio Waves, Source, Origin, Formation, Voyager Missions, Observations, Hectometer Waves, Wavelengths

Scientific paper

Certain Jovian radio emissions seem to be triggered from outside, by much weaker radio waves from the sun. Recently found in the Voyager observations near Jupiter, such triggering occurs at hectometric wavelengths during the arrival of solar radio bursts, with the triggered emissions lasting sometimes more than an hour as they slowly drifted toward higher frequencies. Like the previous discovery of similar triggered emissions at the earth, this suggests that Jupiter's emissions might also originate from natural radio lasers.

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