Synchrotron radiation from a magnetically confined nonneutral hot-electron plasma

1973 ◽  
Vol 16 (4) ◽  
pp. 502 ◽  
Author(s):  
S. F. Nee
1978 ◽  
Vol 21 (11) ◽  
pp. 2038 ◽  
Author(s):  
N. C. Luhmann ◽  
A. W. Trivelpiece

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.


1974 ◽  
Vol 16 (3) ◽  
pp. 275-282 ◽  
Author(s):  
D R Nicholson ◽  
M J Schwartz

1987 ◽  
Vol 63 (9) ◽  
pp. 773-778 ◽  
Author(s):  
J.L. Carrillo ◽  
G. Luna-Acosta ◽  
J. Arriaga ◽  
M.A. Rodríguez

1982 ◽  
Vol 27 (3) ◽  
pp. 507-514
Author(s):  
Bhimsen K. Shivamoggi

For slowly varying wave trains in a linear system, it is known that a quantity proportional to the square of the amplitude propagates with the group velocity. It is shown here, by considering a specific problem of longitudinal waves in a hot electron-plasma and using an asymptotic analysis, that this result continues to be valid even when weak nonlinearities are introduced into the system provided they produce slowly varying wave trains. The method of analysis fails, however, for weakly nonlinear ion-acoustic waves.


1966 ◽  
Vol 9 (4) ◽  
pp. 820 ◽  
Author(s):  
Nicholas A. Krall
Keyword(s):  

1971 ◽  
Vol 27 (2) ◽  
pp. 90-92 ◽  
Author(s):  
D. G. S. Greene ◽  
J. L. Shohet ◽  
P. A. Raimbault
Keyword(s):  

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