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Damping of nonlinear magneto-acoustic waves

Published online by Cambridge University Press:  13 March 2009

G. L. Kalra
Affiliation:
Department of Physics and Astrophysics, University of Delhi, Delhi-110007, India
V. B. Bhatia
Affiliation:
Department of Physics and Astrophysics, University of Delhi, Delhi-110007, India

Abstract

Nonlinear magneto-acoustic waves in a turbulent plasma are simulated by collisional MHD equations. Damping of these waves due to electrical conductivity arising from micro-instabilities and collisional viscosity are analyzed. Numerical investigation of competing effects due to non-linearity and dissipation has been carried out. It is found that finite amplitude perturbation leads to the formation of a shock in both the slow and the fast mode propagation. Collisional viscosity plays an important role in the damping of nonlinear magneto-acoustic waves in the astrophysical and space plasmas.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1978

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References

REFERENCES

Adam, J. A. 1975 Astrophys. Space Sci. 36, 479.CrossRefGoogle Scholar
Lighthill, M. J. 1956 Surveys in Mechanics (Ed. Batchelor, G. K. and Davies, R. M.). Cambridge University Press.Google Scholar
Sakai, J. 1972 Cosmic Electrodyn. 3, 260.Google Scholar
Taniuti, T. & Wet, C. C. 1968 J. Phys. Soc. Japan, 24, 941.CrossRefGoogle Scholar