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Temperature effects in non-symmetric three-component counter-streaming electron plasmas: theory and computer simulation experiments

Published online by Cambridge University Press:  13 March 2009

S. Cuperman
Affiliation:
Department of Physics and Astronomy, Tel-Aviv University, Ramat-Aviv, Israel
M. Mond
Affiliation:
Department of Physics and Astronomy, Tel-Aviv University, Ramat-Aviv, Israel
I. Roth
Affiliation:
Department of Physics and Astronomy, Tel-Aviv University, Ramat-Aviv, Israel
L. Gomberoff
Affiliation:
Department of Physics and Astronomy, Tel-Aviv University, Ramat-Aviv, Israel

Abstract

Temperature effects on the electrostatic instability of non-symmetric electron plasma systems consisting of two warm counter-streaming beams and of warm background particles are investigated linearly (analytically and numerically) and nonlinearly (by computer simulation experiments) for the case of Heaviside and moderately warm Maxwellian particle distribution functions. The non-symmetry is due to unequal temperatures, streaming velocities and particle densities in the beams. Other variable parameters investigated are the relative thermal velocities of the beams and background as well as the relative background particle concentration. When the beam temperatures are unequal, unstable waves with Re ω > 0 and propagating in the direction of the beam with lower temperature occur; this is in contrast to the equal temperature symmetric two-stream case, in which the unstable waves have Re ω = 0 (standing waves) and the temperature effect is only to decrease the growth rate. When three warm components are present in the system, the following results hold: (i) the beam temperatures have the effect of decreasing the importance of the unstable standing waves with Re ω > 0 (and growth rate yB) relative to the waves with Re w = 0 (growth rate yA) which occur in cold three-component symmetric systems; in addition to this, both γA, max and γB, max decrease with increasing temperature; (ii) the background temperature has the general effect of reducing the absolute maximum growth rate. For relative background temperatures above a certain critical value, a separation (in k and ω spaces) of regions B and A occurs; γA, max increases and γB, max decreases with increasing relative background temperature.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1978

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References

REFERENCES

Ackerson, K. L. & Frank, L. A. 1972 J. Geophys. Res. 77, 1128.CrossRefGoogle Scholar
Cuperman, S. & Mond, M. 1976 J. Plasma Phys. 16, 103.CrossRefGoogle Scholar
Cuperman, S., Gomberoff, L. & Roth, I. 1978 J. Plasma Phys. 19, 449.Google Scholar
McIlwain, C. E. 1975 Physics of the Hot Plasma in the Magnetosphere (Ed. Huiquist, B. and Stenflo, L.), p. 91. Plenum.CrossRefGoogle Scholar
Nakai, S., Imasaki, K. & Yamanaki, C. 1977 Plasma Physics and Controlled Nuclear Fusion Research, Nucl. Fusion Supplement, p. 207.Google Scholar