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Electron cyclotron resonance heating of weakly relativistic plasmas

Journal Article · · Phys. Fluids; (United States)
DOI:https://doi.org/10.1063/1.863986· OSTI ID:6789176
Electron cyclotron resonance heating of magnetically confined plasmas is examined with a new formalism which allows convenient evaluation of wave energy deposition in electron energy and momentum spaces, as well as in real space. The formalism applies to wave propagation in general directions in a weakly relativistic plasma. The special case of wave perpendicular to the magnetic field is examined analytically and illustrated with numerical case studies. In that analysis, a general magnetic field profile is assumed. For the mirror-type devices, it is shown that, in contrast to tokamak heating, efficient wave absorption is obtainable at electron temperatures as low as a few eV. For the tandem mirror which operates at a very high temperature, it is shown that electron cyclotron resonance heating (ECRH) results in either edge heating or formation of suprathermal electrons in the center. In comparison, it is shown that in the linear magnetic field profile of the tokamak, high electron temperature would actually favor heating of thermal electrons provided the wave is injected from the low magnetic field side.
Research Organization:
Plasma Physics Division, Naval Research Laboratory, Washington, DC 20375
OSTI ID:
6789176
Journal Information:
Phys. Fluids; (United States), Journal Name: Phys. Fluids; (United States) Vol. 26:1; ISSN PFLDA
Country of Publication:
United States
Language:
English