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Three-wave coupling coefficients for magnetized plasmas with pressure anisotropy

Published online by Cambridge University Press:  13 March 2009

G. Brodin
Affiliation:
Department of Plasma Physics, Umeå University, S-90187 Umeå, Sweden
L. Stenflo
Affiliation:
Department of Plasma Physics, Umeå University, S-90187 Umeå, Sweden

Abstract

In order to find the equations for the nonlinear energy exchange between low-frequency waves in magnetized plasmas in the presence of pressure anisotropy, we start from the Chew–Goldberger–Low equations, the isothermal MHD equations, as well as a new hybrid system of equations. The coupling coefficients describing the interaction between two Alfvén waves and one magnetosonic wave as well as the interaction between two magnetosonic waves and one Alfvén wave are deduced.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1989

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References

REFERENCES

Abraham-Shrauner, B. 1967 J. Plasma Phys. 1, 361.CrossRefGoogle Scholar
Brodin, G. & Stenflo, L. 1988 J. Plasma Phys. 39, 277.CrossRefGoogle Scholar
Chew, G. F., Goldberger, M. L. & Low, F. E. 1956 Proc. R. Soc. Lond. A 236, 112.Google Scholar
Hasegawa, A. 1975 Plasma Instabilities and Nonlinear Effects. Springer.CrossRefGoogle Scholar
Kulsrud, R. M. 1983 Handbook of Plasma Physics (ed. Rosenbluth, M. N. & Sagdeev, R. Z.), vol. 1, Basic Plasma Physics 1 (ed. Galeev, A. A. & Sudan, R. N.), p. 115. North-Holland.Google Scholar
Shi, Y., Lee, L. C. & Fu, Z. F. 1987 J. Geophys. Res. 92, 12171.Google Scholar
Shukla, P. K., Yu, M. Y., Rahman, H. U. & Spatschek, K. H. 1984 Phys. Rep. 105, 227.CrossRefGoogle Scholar
Stenflo, J. O. (ed.) 1983 Solar and Stellar Magnetic Fields: Origins and Coronal Effects. Reidel.CrossRefGoogle Scholar