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4 - Waves in a Cold Plasma

Published online by Cambridge University Press:  16 March 2017

Donald A. Gurnett
Affiliation:
University of Iowa
Amitava Bhattacharjee
Affiliation:
Princeton University, New Jersey
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Summary

When a wave propagates through a plasma with a finite temperature the forces acting on a charged particle are Doppler-shifted from their rest-frame frequency by the thermal motion of the particle. Since these Doppler shifts greatly complicate the analysis, in this chapter the temperature is assumed to be zero, so that there are no thermal motions. Hence the term “cold plasma.” Two types of plasmas are analyzed, those with no background magnetic field, and those with a background magnetic field. To further simplify the analysis, the wave amplitudes are assumed to be small, so that the equations of motion can be linearized. The result is a very general solution can for all of the electromagnetic wave modes that can propagate in a cold plasma, plus one purely electrostatic mode, called the electron plasma oscillation. This analysis reveals almost all of the electromagnetic waves that can propagate in a plasma.
Type
Chapter
Information
Introduction to Plasma Physics
With Space, Laboratory and Astrophysical Applications
, pp. 87 - 147
Publisher: Cambridge University Press
Print publication year: 2017

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References

Alfvén, H. 1942. Existence of electromagnetic-hydrodynamic waves. Nature 150, 405.Google Scholar
Allis, W. P. 1959. Waves in Plasmas, Sherwood Conference on Controlled Fusion, April 27–28, 1959, Gatlinburg, TN, p. 32.
Barkhausen, H. 1919. Zwei mit Hilfe der neuen Verstarker entdeckte Ersheinungen. Phys. Z. 20, 401–403.Google Scholar
Benson, R. F. 1982. Stimulated plasma instability and nonlinear phenomena in the ionosphere. Radio Sci. 17(6), 1637–1659.Google Scholar
Brice, N. M., and Smith, R. L. 1965. Lower hybrid resonance emissions. J. Geophys. Res. 78(1), 71–80.Google Scholar
Budden, K. G. 1961. Radio Waves in the Ionosphere: The Mathematical Theory of the Reflection of Radio Waves from Stratified Ionised Layers. London: Cambridge University Press.
Clemmow, P. C., and Mullaly, R. F. 1955. Dependence of the refractive index in magneto-ionic theory on the direction of the wave normal. Physics of the Ionosphere: Rep. Phys. Soc. Conf. London: London Physical Society, p. 340.
Franklin, C. A., and Maclean, M. A. 1969. The design of swept-frequency topside sounders. Proc. IEEE 57, 897–929.Google Scholar
Gurnett, D. A., Shawhan, S. D., Brice, N. M., and Smith, R. L. 1965. Ion cyclotron whistlers. J. Geophys. Res. 70, 1665–1688.Google Scholar
Haselgrove, J. 1955. Ray theory and a new method for ray tracing. Physics of the Ionosphere: Rep. Phys. Soc. Conf. London: London Physical Society, pp. 355–364.
Helliwell, R. A. 1965. Whistlers and Related Ionospheric Phenomena. Stanford, CA: Stanford University Press, p. 103.
Kaplan, W. 1952. Advanced Calculus. Reading, MA: Addision-Wesley, p. 99.
Manchester, R. N., and Taylor, J. H. 1977. Pulsars. San Francisco, CA: Freeman and Company, p. 134.
Poeverlein, H. 1950. Strahlwege von radiowellen in der ionosphere. Z. Angew. Phys. 2(4), 152–160.Google Scholar
Ratcliffe, J. A. 1962. The Magneto-Ionic Theory and its Application to the Ionosphere. London: Cambridge University Press, p. 126.
Stix, T. H. 1992. Waves in Plasmas. New York: American Institute of Physics, p. 343.
Storey, L. R. O. 1953. An investigation of whistling atmospherics. Philos. Trans. R. Soc. London, Ser. A 246, 113–141.Google Scholar
Townsend, J. S. 1992. A Modern Approach to Quantum Mechanics. New York: McGraw-Hill, p. 79.
Tracy, E. R., Brizard, A. J., Richardson, A. S., and Kaufman, A. N. 2014. Ray Tracing and Beyond: Phase Space Methods in Plasma Wave Theory. New York: Cambridge University Press.
Walsh, D., Haddock, T. F., and Schultz, H. F. 1964. Cosmic radio intensities at 1.225 and 2.0 MC measured up to an altitude of 1700 km. Space Sci. 4, 935–959.Google Scholar
Weinberg, S., 1962. Eikonal methods in magnetohydrodynamics. Phys. Rev. 126, 1899–1909.Google Scholar
Goertz, C. K., and Strangeway, R. J. 1997. Introduction to Space Physics, eds. Kivelson, M. G., and Russell, C. T. Cambridge: Cambridge University Press. Originally published in 1995.
Parks, G. K. 1997. Physics of Space Plasmas: An Introduction. Redwood City, CA: Addison-Wesley, Chapter 9. Originally published in 1991.
Stix, T. H. 1992. Waves in Plasmas. New York: American Institute of Physics.
Swanson, D. G. 1989. Plasma Waves. San Diego, CA:Academic Press, Harcourt Brace, Chapter 2.

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