Flux surface mapping and error field measurement for MUSE table top stellarator
POSTER
Abstract
MUSE is the world's first quasi-axisymmetric stellarator constructed with planar circular coils and permanent magnets[1]. System assembly has finished[2] and electron beam mapping of flux surfaces[3] has been conducted to confirm its magnetic topology.
Good nested flux surfaces have been confirmed at different toroidal field(TF) coil currents. Close agreement of the flux surfaces shapes with flux surfaces from VMEC and FIELDLINES at the corresponding TF value has been demonstrated. The $iota$ profile has been measured and
compared to our model by observing low order resonant structures at different TF values.
Magnetic error field Fourier components will be quantified by measuring flux surface shape deviations and low order islands widths. Attempts will be made
to correct these error fields by adjusting the PM holder positions accordingly.
[1] T. Qian, et al, Nucl. Fusion 084001 (2022)
[2] T. Qian, et al, Design and Construction of the MUSE Permanent Magnet Stellarator, accepted for publication by J. Plasma Physics
[3] S. A. Lazerson, et al, Nucl. Fusion 106005 (2016)
Good nested flux surfaces have been confirmed at different toroidal field(TF) coil currents. Close agreement of the flux surfaces shapes with flux surfaces from VMEC and FIELDLINES at the corresponding TF value has been demonstrated. The $iota$ profile has been measured and
compared to our model by observing low order resonant structures at different TF values.
Magnetic error field Fourier components will be quantified by measuring flux surface shape deviations and low order islands widths. Attempts will be made
to correct these error fields by adjusting the PM holder positions accordingly.
[1] T. Qian, et al, Nucl. Fusion 084001 (2022)
[2] T. Qian, et al, Design and Construction of the MUSE Permanent Magnet Stellarator, accepted for publication by J. Plasma Physics
[3] S. A. Lazerson, et al, Nucl. Fusion 106005 (2016)
Presenters
-
Xu Chu
Princeton University
Authors
-
Xu Chu
Princeton University
-
Michael C Zarnstorff
Princeton Plasma Physics Laboratory, Stellarex, Inc.
-
Tony Qian
Princeton University
-
Bruce Berlinger
Princeton Plasma Physics Laboratory
-
Mohammed Haque
Columbia University, Princeton Plasma Physics Laboratory
-
Simeon Salia
Georgia Institute of Technology
-
Eric Zhu
University of California Santa Barbara
-
Yousef Nasr
Princeton Plasma Physics Laboratory, Rutgers University - New Brunswick
-
Daniel J Williams
Princeton Plasma Physics Laboratory, University of Maryland, Baltimore County