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10 - Waves in a Hot Magnetized 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

An extension of the Landau analysis method presented in Chapter 9 is given to waves propagating in hot magnetized plasmas. The analysis presented reveals an entirely new category of both electrostatic and electromagnetic waves that propagate near harmonics of the electron and ion cyclotron frequencies. These waves are called “Bernstein modes.” For certain types of velocity distribution functions these and other previously analyzed modes, such the whistler mode, can become unstable. Especially notable for being unstable are velocity distribution functions that are rotationally anisotropic with respect to the static magnetic field, such as the loss cone in a planetary radiation belt. Such waves often cause violations of the adiabatic invariants (as in Chapter 3), and cause pitch-angle scattering that leads to the loss of particles from planetary radiation belts. Similar processes also occur for magnetically confined laboratory plasmas.
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Chapter
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Introduction to Plasma Physics
With Space, Laboratory and Astrophysical Applications
, pp. 378 - 427
Publisher: Cambridge University Press
Print publication year: 2017

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