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Experiments on whistler mode electron-cyclotron resonance plasma startup and heating in an axisymmetric magnetic mirror

Journal Article · · Phys. Fluids; (United States)
DOI:https://doi.org/10.1063/1.865353· OSTI ID:5366321
Whistler mode electron-cyclotron resonance heating (ECRH) has been performed simultaneously with whistler mode electron-cyclotron emission measurements on an axisymmetric magnetic mirror plasma. Results presented include a study of the early plasma startup phase and two instability phases, one believed to be caused by a whistler instability and another by magnetohydrodynamic (MHD) flute instability. Enhanced microwave emission at frequencies below the midplane electron-cyclotron frequency has been correlated with enhanced electron endloss during the whistler instability. Cyclotron emission spectra during the startup phase match predictions for a ''sloshing electron'' type distribution based on numerical modeling. This distribution also agrees with anisotropic distributions resulting from electron-cyclotron heating as predicted by Fokker--Planck computer simulations. Experimentally measured heating rates show good agreement with simplified analytical models based on stochastic heating.
Research Organization:
College of Engineering, University of Michigan, Ann Arbor, Michigan 48109
OSTI ID:
5366321
Journal Information:
Phys. Fluids; (United States), Journal Name: Phys. Fluids; (United States) Vol. 28:10; ISSN PFLDA
Country of Publication:
United States
Language:
English