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Electron-cyclotron maser emission from the planets and the starsAuroral kilometric radiation (AKR), Jupiter's decametric radio emission, microwave spike bursts from the Sun, and related bursts from flare stars and close binaries are discussed. Although all of these are produced by the same instability, the plasma conditions in the source regions differ; for the planets the ratio of the plasma frequency to the electron-cyclotron frequency is less than 1, whereas for the Sun and stars it is greater than or = 1. It is shown that as the ratio increases the frequency of the emissions moves to higher harmonics of the electron-cyclotron frequency and the mode changes from electromagnetic to electrostatic. Implications for AKR, microwave spike bursts, and related bursts from the stars are discussed.
Document ID
19870007277
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Winglee, R. M.
(California Univ. Los Angeles, CA, United States)
Dulk, G. A.
(California Univ. Los Angeles, CA, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1986
Publication Information
Publication: CNES Proceedings of a Conference on the Comparative Study of Magnetospheric Systems
Subject Category
Space Sciences (General)
Accession Number
87N16710
Funding Number(s)
CONTRACT_GRANT: NAGW-91
CONTRACT_GRANT: NAGW-78
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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