Features of the Spectra of Oscillations Excited in a Magnetoactive Plasma

Author(s):  
A.N. Antonov ◽  
◽  
V.A. Buts ◽  
Keyword(s):  
1966 ◽  
Vol 89 (6) ◽  
pp. 227-258 ◽  
Author(s):  
A.G. Sitenko ◽  
Yu.A. Kirochkin
Keyword(s):  

1969 ◽  
Vol 11 (9) ◽  
pp. 707-714 ◽  
Author(s):  
N M El-Siragy ◽  
V I Pakhomov

1969 ◽  
Vol 47 (7) ◽  
pp. 757-768 ◽  
Author(s):  
P. C. W. Fung

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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