Bulletin of the American Physical Society
65th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 30–November 3 2023; Denver, Colorado
Session UO06: MFE: Stellarators
2:00 PM–5:00 PM,
Thursday, November 2, 2023
Room: Governor's Square 15
Chair: Eduardo Rodriguez, Max Planck Institute for Plasma Physics - Greifswald
Abstract: UO06.00010 : Global gyrokinetic simulations of electrostatic microturbulent transport in LHD stellarator with boron impurity*
3:48 PM–4:00 PM
Presenter:
Tajinder Singh
(Department of Physics, Indian Institute of Science, Bangalore 560012, India)
Authors:
Tajinder Singh
(Department of Physics, Indian Institute of Science, Bangalore 560012, India)
Javier H. Nicolau
(Department of Physics and Astronomy, University of California, Irvine, California 92697, USA)
Federico Nespoli
(Princeton Plasma Physics Laboratory, Princeton, NJ 08540, USA)
Gen Motojima
(National Institute for Fusion Science, National Institutes of Natural Sciences, 322-6 Oroshi-cho, Toki, Gifu 509-5292, Japan)
Zhihong Lin
(Department of Physics and Astronomy, University of California, Irvine, California 92697, USA)
Abhijit Sen
(Institute for Plasma Research, Bhat, Gandhinagar 382428, India)
Sarveshwar Sharma
(Institute for Plasma Research, Bhat, Gandhinagar 382428, India)
Animesh Kuley
(Department of Physics, Indian Institute of Science, Bangalore 560012, India)
Collaboration:
The authors thank Xishuo Wei and Walter Guttenfelder for the helpful discussion.
*This work is supported by the National Supercomputing Mission (Ref No: DST/NSM/R&D HPC Applications/2021/4), Board of Research in Nuclear Sciences (BRNS Sanctioned No. 57/14/04/2022-BRNS), Science and Engineering Research Board EMEQ program (SERB sanctioned no. EEQ/2022/000144). A.S. thanks the Indian National Science Academy (INSA) for their support under the INSA Senior Scientist Fellowship scheme. This work was conducted within the framework of the NIFS/PPPL International Collaboration and it is supported by the US DOE under Contract No. DE-AC02-09CH11466 with Princeton University. This work was partially supported by the US Department of Energy under Award No. DE-SC0018270 (SciDAC ISEP Center) and DE-FG02-07ER54916. This work has used the resources of the Param Pravega supercomputer at the Indian Institute of Science, Bangalore, India.
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