Experimental Observation of an Unstable Mode in Theoretically Ideal MHD Stable Plasmas Confined in the L-2M Stellarator
- Autores: Shchepetov S.V.1, Vasilkov D.G.1,2, Kholnov Y.V.1
- 
							Afiliações: 
							- Prokhorov General Physics Institute
- Bauman Moscow State Technical University
 
- Edição: Volume 44, Nº 6 (2018)
- Páginas: 539-543
- Seção: Stellarators
- URL: https://journal-vniispk.ru/1063-780X/article/view/186778
- DOI: https://doi.org/10.1134/S1063780X18060090
- ID: 186778
Citar
Resumo
In net-free current plasmas that are confined in the L-2M stellarator, an electromagnetic mode having thresholds in the plasma density and pressure was observed. The characteristic frequency of the unstable mode was 70–90 kHz, and the direction of its rotation pointed toward the direction of ion diamagnetic drift. The instability was observed at n(0) > 1.5 × 1013 cm-3 and 〈β〉 > 0.14%, where n(0) is the plasma density averaged over the central chord and 〈β〉 is volume-averaged ratio of the gas kinetic pressure to the magnetic pressure. This phenomenon cannot be described within the theory of resistive interchange modes. Possible reasons for the occurrence of the observed electromagnetic mode are discussed using analytical estimations.
Sobre autores
S. Shchepetov
Prokhorov General Physics Institute
							Autor responsável pela correspondência
							Email: shch@fpl.gpi.ru
				                					                																			                												                	Rússia, 							Moscow, 119991						
D. Vasilkov
Prokhorov General Physics Institute; Bauman Moscow State Technical University
														Email: shch@fpl.gpi.ru
				                					                																			                												                	Rússia, 							Moscow, 119991; Moscow, 105005						
Yu. Kholnov
Prokhorov General Physics Institute
														Email: shch@fpl.gpi.ru
				                					                																			                												                	Rússia, 							Moscow, 119991						
Arquivos suplementares
 
				
			 
						 
						 
						 
						 
					 
				 
  
  
  
  
  Enviar artigo por via de e-mail
			Enviar artigo por via de e-mail  Acesso aberto
		                                Acesso aberto Acesso está concedido
						Acesso está concedido Somente assinantes
		                                		                                        Somente assinantes
		                                					