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Stability of a stratified partially ionized plasma in a vertical magnetic field

Published online by Cambridge University Press:  13 March 2009

S. L. Maheshwari
Affiliation:
Department of Mathematics, University of Jodhpur, Jodhpur, India
P. K. Bhatia
Affiliation:
Department of Mathematics, University of Jodhpur, Jodhpur, India

Abstract

The dynamic stability of a stratified layer of partially ionized compressible plasma is discussed to investigate the effects of finite electrical conductivity and ion viscosity. The prevailing magnetic field is assumed to be uniform and vertical. For a semi-infinite plasma having a one-dimensional exponential density gradient along the vertical, the dispersion relation has been obtained by variational methods. It is found that the ion viscosity and ion–neutral collisions, whether included jointly or separately, do not change the stability criterion of the perfectly conducting system. Their inclusion, however, has a tendency to reduce the growth rate of the unstable perturbations showing that they have a stabilizing influence. On the other hand the inclusion of the effects of finite resistivity and compressibility of the medium is found to be destabilizing as the wavenumber range over which the plasma would otherwise be stable, becomes unstable.

Type
Research Article
Copyright
Copyright © Cambridge University Press 1978

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References

REFEREMCES

Alfvén, H. 1954 On the Origin of the Solar System. Oxford Univeisity Press.Google Scholar
Ariel, P. D. 1971 Appl. Sci. Res. 24, 294.CrossRefGoogle Scholar
Bhatia, P. K. 1974 Astrophys. and Space Sci. 26, 319.CrossRefGoogle Scholar
Chandrasekhar, S. 1961 Hydroclynamic and Hydromagnetic Stability. Clarendon.Google Scholar
Lehnert, B. 1959 Nuovo Cimento Suppl. A 13(10), 59.CrossRefGoogle Scholar
Lehnert, B. 1969 Roy. Inst. of Technology, Stockholm, Rep. 69–25.Google Scholar
Lehnert, B. 1970 Cosmic Electrodyn. 1, 397.Google Scholar
Lehnert, B. 1972 Roy. Inst. of Technology, Stockholm, Reps. TRITA-EPP.72–05, TRITA-EPP-72.06 and Proc. Fifth European Conf. on Controlled Fusion and Plasma Phys., Grenoble,Google Scholar
Piddington, J. H. 1954 Mon. Not. Roy. Astron. Soc. 14, 638, 651.CrossRefGoogle Scholar
Rayleigh, , Lord, 1883 Proc. London Math. Soc. 14, 170.Google Scholar
Sharma, B. M. & Ariel, P. D. 1975 Proc. natn. Acad. Sci. India 45 (A), 241.Google Scholar
Strömgren, B. 1939 Astrophys. J. 89, 526.CrossRefGoogle Scholar