An upper limit for the 34.3-MHz synchrotron flux from Uranus

Details An upper limit for the 34.3-MHz synchrotron flux from Uranus An upper limit for the 34.3-MHz synchrotron flux from Uranus

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jgr....82.1947s&link_type=abstract

Journal of Geophysical Research, vol. 82, May 1, 1977, p. 1947-1950.

Astronomy and Astrophysics

Astronomy

1

Planetary Radiation, Synchrotron Radiation, Uranus (Planet), Astronomical Catalogs, Frequency Response, Long Wave Radiation, Radio Astronomy, Radio Telescopes

Scientific paper

The 34.3-MHz Cocoa Cross radio telescope at Clark Lake Radio Observatory has been used to search for synchrotron radiation from Uranus between November 27, 1974, and May 13, 1975. Inspection of daily chart records for 69 observations during this time period provides a conservative upper limit to the synchrotron flux of 8 Jy. No Uranian bursts were observed. This result is compared with the kilometric burst observations of Brown (1976) as well as with models for burst and possible synchrotron emission from Uranus.

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