Possible radio emission from Uranus at 0.5 MHz

Details Possible radio emission from Uranus at 0.5 MHz Possible radio emission from Uranus at 0.5 MHz

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7616008b&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Explorer 43 Satellite, Radio Emission, Uranus (Planet), Radio Bursts, Satellite Observation, Signal Detection

Scientific paper

Radio emission from the direction of Uranus was detected in data from the radio astronomy experiment on the IMP-6 spacecraft. Previously, emission from the direction of Jupiter and Saturn was observed by the IMP-6 at a number of frequencies near 1 MHz during the period April 1971 to October 1972. These radio bursts were identified in the IMP-6 data through an analysis of the phase of the observed modulated signal detected from the spinning dipole antenna. This technique was applied to the direction of the planet Uranus with possible positive results. Over the approximately 500 days of data, three to six bursts with unique spectral characteristics were found. Identification with Uranus is confused by the likely presence of low level terrestrial and solar emission. The observed events persisted less than three minutes and are strongest in intensity near 0.5 MHz.

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