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28 GHZ EBW HEATING, CURRENT DRIVE AND EMISSION EXPERIMENTS AT THE WEGA STELLARATOR

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    0360903 - ÚFP 2012 RIV SG eng C - Conference Paper (international conference)
    Laqua, H.P. - Chlechowitz, E. - Glaubitz, M. - Marsen, S. - Stange, T. - Otte, M. - Zhang, D. - Preinhaelter, Josef - Urban, Jakub
    28 GHZ EBW HEATING, CURRENT DRIVE AND EMISSION EXPERIMENTS AT THE WEGA STELLARATOR.
    Electron Cyclotron Emission and Electron Cyclotron Resonance Heating (EC-16):Proceedings of the 16th Joint Workshop. Toh Tuck Link: World Scientific, 2011, s. 263-268. ISBN 978-981-4340-26-7.
    [Joint Workshop on Electron Cyclotron Emission and Electron Cyclotron Resonance Heating/16th./. Sanya (CN), 12.04.2010-15.04.2010]
    R&D Projects: GA MŠMT 7G10072; GA MŠMT LA08048; GA ČR GA202/08/0419
    Institutional research plan: CEZ:AV0Z20430508
    Keywords : Stellarator * Electron Bernstein wave * EBW * WEGA * ECRH
    Subject RIV: BL - Plasma and Gas Discharge Physics

    This paper reports on detailed investigation of a fully 28 GHz EBW (electron Bernstein wave) heated plasma in the WEGA stellarator. The plasma shows a fast transition into the “OXB-state” when the threshold density is reached. The profiles become peaked. The EBW emission diagnostic measures a radiation temperature of several keV, which origins from a supra-thermal electron population. The angular dependence of the mode conversion could be confirmed with a movable launching mirror. The toroidal current and the plasma conductivity were measured for different microwave launch positions.
    Permanent Link: http://hdl.handle.net/11104/0198345

     
     
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