Observations of Jupiter at 26.3 MHz using a large array

Details Observations of Jupiter at 26.3 MHz using a large array Observations of Jupiter at 26.3 MHz using a large array

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icar...25...12d&link_type=abstract

Icarus, vol. 25, May 1975, p. 12-17. NSF-NASA-supported research.

Astronomy and Astrophysics

Astronomy

9

Dipole Antennas, Io, Jupiter (Planet), Planetary Radiation, Antenna Arrays, Astronomical Maps, High Frequencies, Phase Modulation, Radio Emission, Radio Sources (Astronomy), Steerable Antennas

Scientific paper

A 640 element phase-steerable dipole array has been used to make highly sensitive observations of the planet Jupiter during the 1973 apparition. The satellite Io is found to have very little influence at the low flux levels, whereas the definition of sources A and B appears to be relatively flux independent. A two-dimensional analysis of the data in the Jupiter-Io plane has revealed considerable source B activity at low intensities which is not influenced by Io.

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