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 CP11: Poster Session II: Basic Plasma Physics; Boundary, PMI, Proto-MPEX; International Tokamaks; Turbulence and Transport; Other Configurations; Z-pinch, Dense Plasma Focus and MagLIF (2:00pm-5:00pm)
Monday, November 5, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.CP11.114
Abstract: CP11.00114 : Study of argon impurity transport by X-ray imaging crystal spectrometer on J-TEXT*
Presenter:
Wei Yan
(Huazhong University of Science and Technology)
Authors:
Wei Yan
(Huazhong University of Science and Technology)
Zhongyong chen
(Huazhong University of Science and Technology)
Xiaolong Zhang
(Shenzhen University)
Zhifeng Cheng
(Huazhong University of Science and Technology)
Rui hai Tong
(Huazhong University of Science and Technology)
Yunong Wei
(Huazhong University of Science and Technology)
Zhifang Lin
(Huazhong University of Science and Technology)
A tangential X-ray imaging crystal spectrometer (XICS) has been designed to receive emissions of Ar XVII from −13 cm to +13 cm region with a spatial resolution of 1.8 cm in the vertical direction on J-TEXT. The temporal evolution of argon impurity density profiles after an argon gas puff could be observed with a time resolution of up to 2 ms. The emissions of Ar XVII can be modulated by the resonant magnetic perturbations (RMPs) which indicates that the transport of argon is affected by the RMPs significantly. The 2/1 RMPs can lead to field penetration with enough RMPs amplitude. The XICS provides a tool for the study of the transport of argon impurities during the penetration of RMPs. During the field penetration phase, the emissions of Ar XVII decreased. The phenomena show that the transport of argon impurity in the core region has been enhanced during the field penetration phase. STRAHL can give the ratio between D and v profiles for the argon. The result shows that the argon is moving towards the core by the convection.
*the National Natural Science Foundation of China (Nos. 11775089, 71762031); the National Magnetic Confinement Fusion Science Program (Nos. 2015GB111002, 2014GB118000).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.CP11.114
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