Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session PO5: Boundary, Plasma Materials Interactions, Stellarators
2:00 PM–5:00 PM,
Wednesday, November 7, 2018
OCC
Room: B113-114
Chair: Oliver Schmitz, University of Wisconsin
Abstract ID: BAPS.2018.DPP.PO5.15
Abstract: PO5.00015 : Predicting Equilibrium Electron Density Production on Proto-MPEX*
4:48 PM–5:00 PM
Presenter:
Pawel Andrzej Piotrowicz
(Univeristy of Illinois - Urbana)
Authors:
Pawel Andrzej Piotrowicz
(Univeristy of Illinois - Urbana)
Juan F Caneses
(Oak Ridge National Lab)
Nischal Kafle
(Univ of Tennessee, Knoxville)
Richard H Goulding
(Oak Ridge National Lab)
David L Green
(Oak Ridge National Lab)
John B Caughman
(Oak Ridge National Lab)
Cornwall Hong Man Lau
(Oak Ridge National Lab)
David Neil Ruzic
(Univeristy of Illinois - Urbana)
The helicon antenna plasma source installed on Proto-MPEX has been able to produce electron densities of ne >6×1019 m-3 in the “helicon-mode”. The existing power availability of the helicon antenna is P≈100 kW at 13.56 MHz driving frequency. The “helicon-mode” plasma on Proto-MPEX is only observed up to a magnetic field of BH < 0.08 T. This low operating magnetic field strength restricts the plasma diameter at the target, which is typically operated at B0 ≈ 1.0 T, to dp ≈ 4 cm. A larger plasma diameter would be beneficial to Proto-MPEX both for electron and ion heating demonstration as well as future PMI experiments. A full-wave electromagnetic model that was used to explain the mechanisms that lead to the observation of the “helicon-mode” plasma on Proto-MPEX is used to predict power deposition in the helicon region. Power losses are calculated and used in a power balance to predict an equilibrium electron density. Comparison with experimentally measured electron density variation with magnetic field strength at a power level of P = 100 kW is presented. This model is then used to predict the expected electron density at higher magnetic field values with an available power of P = 200 kW.
*This work is supported under Contract No. DE-AC05- 00OR22725 with the U.S. DOE.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.PO5.15
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