Synchrotron radiation from single electrons gyrating in a magnetoactive plasma
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The Past
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In this paper, the incoherent synchrotron radiation power emitted by relativistic electrons gyrating in a cold magnetoactive plasma is rederived, correcting errors which have occurred in the past literature. One can specify the background plasma by the quantity A = ωp2/ωH2 (ωp is the angular electron plasma frequency and ωH is the angular electron gyro-frequency), i.e. the relative importance of the plasma frequency to the gyro-frequency. The general spectral features of synchrotron radiation from single electrons radiating in plasmas of large [Formula: see text] and small [Formula: see text] are discussed with the aid of a number of numerical examples.
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2016 ◽
Vol 13
(4)
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pp. 315-327
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2007 ◽
Vol 73
(3)
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pp. 315-330
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2000 ◽
Vol 105
(A6)
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pp. 12919-12927
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2021 ◽
Vol 4
(2.2)
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pp. 120-127
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1988 ◽
Vol 268
(1)
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pp. 262-269
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