Groundbased and spacecraft studies of Jupiter at decameter and hectometer wavelengths

Details Groundbased and spacecraft studies of Jupiter at decameter and hectometer wavelengths Groundbased and spacecraft studies of Jupiter at decameter and hectometer wavelengths

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976phdt.........9d&link_type=abstract

Ph.D. Thesis Florida Univ., Gainesville.

Astronomy and Astrophysics

Astronomy

6

Explorer 38 Satellite, Ground Stations, Jupiter (Planet), Radio Emission, Flux Density, Radio Frequencies, Radiometers

Scientific paper

The low frequency Jovian emission between 450 kHz and 26.3 MHz has provided information on a component of Jovian emission which is three orders of magnitude weaker than that detected with conventional radiometer systems. Deployment of the earth orbiting Radio Astronomy Explorer 1 satellite was used to identify Jovian activity at eight frequencies between 450 and 6550 kHz. Both the ground based and spacecraft systems are described, as are the procedures which were developed to obtain their absolute effective apertures and pointing directions.

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