Measurement of an upper limit on the flux density of radio emission from Saturn at 102.5 MHz

Details Measurement of an upper limit on the flux density of radio emission from Saturn at 102.5 MHz Measurement of an upper limit on the flux density of radio emission from Saturn at 102.5 MHz

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..373k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, Aug. 1977, p. 373-375. In Russian.

Astronomy and Astrophysics

Astronomy

Brightness Temperature, Planetary Radiation, Radio Astronomy, Radio Emission, Saturn (Planet), Very High Frequencies, Data Processing, Jupiter (Planet), Radiant Flux Density, Radio Telescopes, Synchrotron Radiation

Scientific paper

Results are reported for radio observations of Saturn carried out at a frequency of 102.5 MHz (wavelength of 2.92 m). No radio emission from Saturn was detected at this frequency, but upper limits of 0.1 Jy and 50,000 K are placed on the flux density and brightness temperature, respectively. The upper limit on the 102.5-MHz flux density is shown to be at least an order of magnitude lower than the value to be expected if Saturn were the same kind of synchrotron-radiation source as Jupiter.

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