Two-Dimensional Distribution of Plasma Electric Potential in the T-10 Tokamak
- Autores: Ammosov Y.M.1,2, Khabanov F.O.3, Drabinskiy M.A.1, Melnikov A.V.1,2,4, Eliseev L.G.1, Kharchev N.K.1,5, Lysenko S.E.1
- 
							Afiliações: 
							- National Research Centre “Kurchatov Institute”
- Moscow Institute of Physics and Technology (National Research University)
- University of Wisconsin-Madison
- National Research Nuclear University “Moscow Engineering Physics Institute”
- Prokhorov General Physics Institute, Russian Academy of Sciences
 
- Edição: Volume 49, Nº 10 (2023)
- Páginas: 947-952
- Seção: TOKAMAKS
- URL: https://cardiosomatics.ru/0367-2921/article/view/668430
- DOI: https://doi.org/10.31857/S0367292123600656
- EDN: https://elibrary.ru/EPYZPV
- ID: 668430
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Texto integral
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						Acesso está concedido Acesso é pago ou somente para assinantes
		                                							Acesso é pago ou somente para assinantes
		                                					Resumo
Heavy ion beam probe (HIBP) is a unique plasma diagnostics that makes it possible to measure the electric potential φ of high-temperature plasma and its fluctuations y, as well as the density ne and poloidal magnetic field Bpol fluctuations. Position of the point of performing measurements in the plasma vertical cross-section depends on the beam energy and angle of its entrance into the plasma. The variation of these two parameters makes it possible to construct a two-dimensional (2D) detector grid, which covers the domain of possible measurements. The measurement results obtained in the detector grid points provide for constructing 2D distributions of plasma parameters. For the OH and ECRH stages of the T-10 tokamak shots, 2D distributions of the plasma electric potential are presented for the regime with the on-axis magnetic field of Bt = 2.2 T, plasma current of Ipl = 230 kA, line-average density of ne ≈ 1.1 × 1019 m–3 and off-axis ECRH power of PECRH = 1.7 MW.
Sobre autores
Ya. Ammosov
National Research Centre “Kurchatov Institute”; Moscow Institute of Physics and Technology (National Research University)
														Email: ammosov.ium@phystech.edu
				                					                																			                												                								123182, Moscow, Russia; 141701, Dolgoprudny, Russia						
F. Khabanov
University of Wisconsin-Madison
														Email: melnikov_07@yahoo.com
				                					                																			                												                								53706, Madison, WI, USA						
M. Drabinskiy
National Research Centre “Kurchatov Institute”
														Email: melnikov_07@yahoo.com
				                					                																			                												                								123182, Moscow, Russia						
A. Melnikov
National Research Centre “Kurchatov Institute”; Moscow Institute of Physics and Technology (National Research University); National Research Nuclear University “Moscow Engineering Physics Institute”
														Email: melnikov_07@yahoo.com
				                					                																			                												                								123182, Moscow, Russia; 141701, Dolgoprudny, Russia; 115409, Moscow, Russia						
L. Eliseev
National Research Centre “Kurchatov Institute”
														Email: melnikov_07@yahoo.com
				                					                																			                												                								123182, Moscow, Russia						
N. Kharchev
National Research Centre “Kurchatov Institute”; Prokhorov General Physics Institute, Russian Academy of Sciences
														Email: melnikov_07@yahoo.com
				                					                																			                												                								123182, Moscow, Russia; 119991, Moscow, Russia						
S. Lysenko
National Research Centre “Kurchatov Institute”
							Autor responsável pela correspondência
							Email: melnikov_07@yahoo.com
				                					                																			                												                								123182, Moscow, Russia						
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