NASA NTRS · 19750050980
Observations of Jupiter at 26.3 MHz using a large array
Abstract
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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Desch, M. D., Carr, T. D., Levy, J.. 1975-05-01. Observations of Jupiter at 26.3 MHz using a large array. https://ntrs.nasa.gov/citations/19750050980
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