Electron Bernstein Wave Studies in MST
POSTER
Abstract
The overdense condition in a RFP prevents electromagnetic waves from propagating past the extreme edge. However use of the electron Bernstein wave (EBW) has the potential to heat and drive current in the plasma. MHD simulations have demonstrated that resistive tearing mode stability is very sensitive to the gradient in the edge current density profile, allowing EBW current drive to influence and potentially stabilize tearing mode activity. Coupling between the X-mode and Bernstein waves is strongly dependent on the edge density gradient. The effects on coupling of plasma density, magnetic field strength, antenna radial position and launch polarization have been examined. Coupling as high as 90{\%} has been observed. Construction of a 450kw RF source is complete and initial experimental results will be reported. The power and energy of this auxiliary system should be sufficient for several scientific purposes, including verifying mode conversion, EBW propagation and absorption in high beta plasmas. Target plasmas in the 300-400kA range will be heated near the reversal surface, potentially allowing mode control, while target plasmas in the 250kA range will allow heating near the core, allowing better observation of heating effects. Heating and heat pulse propagation experiments are planned, as well as probing the stability of parametric decay during mode conversion, at moderate injected power.
Authors
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Andrew Seltzman
University of Wisconsin-Madison
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Jay Anderson
University of Wisconsin-Madison, University of Wisconsin, University of Wisconsin - Madison
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Cary Forest
University of Wisconsin, UW-Madison, University of Wisconsin-Madison, University of Wisconsin - Madison
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Paul Nonn
University of Wisconsin-Madison
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Mark Thomas
University of Wisconsin-Madison
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J.A. Reusch
University of Wisconsin-Madison, University of Wisconsin, UW-Madison
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Eric Hendries
University of Wisconsin-Madison