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Changes in Jupiter's 13-cm Synchrotron Radio Emission Following the Impact of Comet Shoemaker-Levy-9Results of an observing program to monitor the synchrotron radio emission from Jupiter's inner radiation belts before, during and after the impact of Comet SL-9 are reported. The observations were made at 2295 MHz as part of the NASA-JPL Jupiter Patrol, a long-term radio astronomy monitoring program begun in 1971. ne data indicate that the intensity of the synchrotron emission at 13 cm wavelength increased by 27 percent within a few days after the comet impacts; the longitudinal beaming curve was distorted during the week of impacts; the magnetic latitude beaming curves flattened after the week of impacts suggesting an increase in the emission at higher magnetic latitudes; and the decay of the enhanced emission is consistent with an exponential with a time constant of approx. 125 days. The reported changes following the SL-9 impact are unprecedented in the 23-year history of the Jupiter Patrol.
Document ID
19990103115
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Klein, M. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Gulkis, S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Bolton, S. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 19, 2013
Publication Date
July 1, 1995
Publication Information
Publication: Geophysical Research Letters
Publisher: American Geophysical Union
Volume: 22
Issue: 13
ISSN: 0094-8534
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
Paper-95GL01415
Distribution Limits
Public
Copyright
Other

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