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Some recent observations and interpretation of the Jupiter decimeter emissionThe decimetric emission consists partly of thermal radiation from the planetary disk and partly of nonthermal radiation from a region of larger angular extent and is thought to result from synchrotron emission by relativistic electrons in the magnetic field. Four topics relating to the decimetric emission are discussed. (1) A comparison is made of maps giving detailed brightness contours. One was obtained for epoch 1963.8 and was at a wavelength of 10.4 cm. The second was for epoch 1967.2 at 21.3 cm. (2) Interferometric data at 21.1 cm taken in April 1968 and May 1979 indicate that the emission centroid is fixed in Jupiter and rotates with it. (3) Circular polarization observations are described and are used to obtain a surface magnetic field strength at the equator between 3.2 and 15.2 gauss. (4) An upper limit on the Faraday rotation is used to set an upper limit on the density of thermal electrons surrounding Jupiter, and uncertainties in the results are discussed.
Document ID
19720020211
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Berge, G. L.
(California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 6, 2013
Publication Date
July 1, 1972
Publication Information
Publication: JPL Proc. of the Jupiter Radiation Belt Workshop
Subject Category
Space Sciences
Accession Number
72N27861
Funding Number(s)
CONTRACT_GRANT: NGR-05-002-114
CONTRACT_GRANT: N00014-67-A-0094-0019
CONTRACT_GRANT: NSF GP-30400X
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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