Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-27T14:27:29.605Z Has data issue: false hasContentIssue false
  • English
  • Français

Characteristics of the fast and slow magnetosonic waves in layered plasmas

Published online by Cambridge University Press:  13 March 2009

Tsutomu Tamao
Tsutomu Tamao
Affiliation:
Geophysics Research Laboratory, University of Tokyo, Tokyo 133, Japan
Get access Rights & Permissions [Opens in a new window]

Abstract

Propagation characteristics of two magnetosonic waves, the fast and slow modes, in layered plasmas with different β values are studied, where β is the ratio of plasma pressure to magnetic pressure. In the first part we consider the efficiency of wave penetration from one region to another with different β ratios, β1 and β2. In particular, the condition for the total reflexion, amplitude and phase of the reflexion and transmission coefficients at the interface are obtained for both modes. The results indicate that the range of deviation of the ratio β2/β1 from unity is very small for penetration of the slow mode, while the ratio for the fast mode covers a wide range. In the second part, the fast and slow normal modes of magnetosonic waves in layered plasmas are discussed and their phase and group velocities, and the spatial damping rate due to partial leakage of wave energy are compared between two modes. From these, it is concluded that the presence of the slow magnetosonic waves is restricted to within the high-β plasma region. Finally, application of these to the earth's magnetosphere is given qualitatively.

Type
Research Article
Information
Journal of Plasma Physics , Volume 9 , Issue 3 , June 1973 , pp. 429 - 442
Copyright
Copyright © Cambridge University Press 1973

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

Coroniti, F. V. & Kennel, C. F. 1972 J. Geophys. Res. 77, 3361.CrossRefGoogle Scholar
Formisano, V. & Kennel, C. F. 1969 J. Plasma Phys. 3, 55.CrossRefGoogle Scholar
Grad, H. 1959 Magnetohydrodynamics of Conducting Fluids (ed. Bershader, D.), p. 37. Stanford University Press.Google Scholar
Hulst, Van De, H. 1951 Problems of Cosmical Aerodynamics, p. 45. Dayton, Ohio: Central Air Document Office.Google Scholar
Kantrowitz, A. R. & Petschek, H. E. 1964 AVCO Res. Rep. 185.Google Scholar
Ness, N. F. 1969 Rev. Geophys. 7, 97.CrossRefGoogle Scholar
Patel, V. L. 1968 Phys. Lett. 26 A, 596.CrossRefGoogle Scholar
Patel, V. L. 1971 IUGG Preprint, Moscow.Google Scholar
Siscoe, G. L. 1969 J. Geophys. Res. 74, 6482.CrossRefGoogle Scholar
Stix, T. H. 1962 The Theory of Plasma Waves. McGraw-Hill.Google Scholar
Stringer, T. E. 1963 J. Nuclear Energy, C 5, 89.CrossRefGoogle Scholar
Tamao, T. 1972 J. Geophys. Res. (To be published.)Google Scholar
Thompson, W. B. 1962 An Introduction to Plasma Physics, p. 79. Pergamon.Google Scholar