Cassini-Jupiter microwave observing campaign: DSN and GAVRT observations of Jovian synchrotron radio emission
This paper discusses the Cassini-Jupiter microwave observing campaign.
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Publications and source records attributed to Klein, M. J..
This paper discusses the Cassini-Jupiter microwave observing campaign.
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Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
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This paper reports the Cassini-JMOC observations supported by NASA's Deep Space Network (DSN) antennas at Goldstone, California.
One objective of the Cassini-Jupiter Microwave Observing Campaign observations was to measure Jupiter's average disk temperature with high accuracy at 13.78 GHz, which is the frequency of the radar receiver on the spacecraft. Preliminary results of the ground-based observations are reported. A second objective of the Cassini-JMOC project included an educational compment that allowed middle- and high school students to participate directly in the ground-based observations and data analysis.
In this paper we discuss recent observations on the study of synchrotron radio emission from Jupiter's inner radiation belts.
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This paper reports supporting ground-based C-JMOC observations made with NASA's Deep Space Network antennas at Goldstone, California.
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