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Microwave absorption in stellarators with a non-Maxwellian electron distribution function

Journal Article · · Physics of Fluids B: Plasma Physics; (USA)
DOI:https://doi.org/10.1063/1.859034· OSTI ID:5350118
;  [1]
  1. Asociacion EURATOM-CIEMAT para la Fusion, Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (C.I.E.M.A.T.), 28040 Madrid, Spain (ES)

The magnetic configurations of two stellarators, ATF (Fusion Technol. {bold 10}, 170 (1986)) and TJ-II (Fusion Technol. {bold 13}, 315 (1986)), are used as examples to study the influence that a superthermal component in the electron distribution function has upon the electron cyclotron resonance heating absorption process for microwaves propagating in the first and second harmonic of the electron cyclotron frequency. The non-Maxwellian tail is simulated by adding a drifting Maxwellian to a bulk distribution function and an analytical form of the weakly relativistic dielectric tensor is obtained. The quantitative, and more importantly, the qualitative differences between nonrelativistic and relativistic models are also presented. A numerical analysis shows that an increase of up to 50% in the absorption power with respect to the pure Maxwellian models, can be obtained if sufficient superthermal populations are present in the plasma.

OSTI ID:
5350118
Journal Information:
Physics of Fluids B: Plasma Physics; (USA), Journal Name: Physics of Fluids B: Plasma Physics; (USA) Vol. 1:11; ISSN 0899-8221; ISSN PFBPE
Country of Publication:
United States
Language:
English