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NASA NTRS ยท 19840043273

Parametric instabilities during electron cyclotron heating of tandem mirrors

Abstract

Electron cyclotron resonance heating is one of the most commonly used methods of heating electrons in the plugs and in the thermal barriers of tandem mirrors. The intense coherent electromagnetic waves used for such heating are susceptible to parametric decay into other modes. Significant growth rates are found for the decay of either ordinary or extraordinary waves into two magnetized electron plasma waves. This and related effects may result in electron heating mechanisms rather different than those assumed in linear ray-tracing calculations. These results may help explain the unusual effects observed during heating of the Phaedrus tandem mirror device. In the general case, these instabilities may be strongly inhibited by density gradients.

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BibTeXRIS

Nicholson, D. R.. 1984-03-01. Parametric instabilities during electron cyclotron heating of tandem mirrors. https://ntrs.nasa.gov/citations/19840043273

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