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 JP11: Poster Session IV: Education and Outreach; Undergraduate or High School Research; Plasma technology, Fusion reactor Nuclear and Materials Science; Propulsion; Materials Interfaces (2:00pm-5:00pm)
Tuesday, November 6, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.JP11.34
Abstract: JP11.00034 : Misalignment of magnetic field in DIII-D assessed by post mortem analysis of divertor targets*
Presenter:
Rebecca Masline
(UCSD)
Authors:
Rebecca Masline
(UCSD)
Igor Bykov
(Univ of California - San Diego)
Dmitriy M Orlov
(Univ of California - San Diego)
Jerome Guterl
(ORAU, Oak Ridge, TN, USA)
Richard A Moyer
(Univ of California - San Diego)
Todd E Evans
(General Atomics - San Diego)
Huiqian Wang
(ORAU, Oak Ridge, TN, USA)
John Watkins
(SNL)
Eric Matthias Hollmann
(Univ of California - San Diego)
We assess the magnetic field toroidal asymmetry in DIII-D present due to a misalignment of the toroidal field coils with respect to the vessel structure. The peak-to-peak variation of the radial strike point (SP) location is measured to be 1.0 cm, with n=1 toroidal pattern. We use the center of a narrow C deposition band present on tungsten-coated divertor tiles just inside the outer SP as a proxy for the magnetic strike point location. The band occurred in a series of rev. Bt discharges during the Metal Rings Campaign due to strong ExB drift transport of C from the inner to the outer SP through the private flux region. The variation in band radius (and hence the magnetic SP) will be compared to measurements of the 3D magnetic field distribution [1], simulations performed by the TRIP3D field line tracing code, and recent Langmuir probe measurements in the Small-Angle-Slot (SAS) divertor [2]. These studies will be important for better understanding the radial variation of the toroidal strike line in DIII-D and for designing the new generation of the SAS divertor.
[1] M. Schaffer, et al, Bull. Am. Phys. Soc. 52, 164 (2007)
[2] J.G. Watkins et al., PSI-23
*This work supported by the US Department of Energy under DE-FG02-07ER54917, DE-SC0018030, DE-NA0003525, DE-FC02-04ER54698
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.JP11.34
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