TJ-II: Density limit and ZFs in TJ-II: Difference between revisions

(Created page with "== Experimental campaign == 2020 Spring == Proposal title == '''TJ-II: Density limit and ZFs in TJ-II''' == Name and affiliation of proponent == Ulises Losada, Daniel Ferná...")
 
 
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Density limit is manifested in tokamaks, stellarators and RFPs. In stellarator the density limit is related to radiation collapse mechanisms <ref>M. Hirsch et al., PPCF 2007)</ref> whereas in tokamaks edge transport can play an important role <ref>M. Greenwald Plasma Phys. Control. Fusion 44 (2002) R27</ref>.  
Density limit is manifested in tokamaks, stellarators and RFPs. In stellarator the density limit is related to radiation collapse mechanisms <ref>M. Hirsch et al., PPCF 2007)</ref> whereas in tokamaks edge transport can play an important role <ref>M. Greenwald Plasma Phys. Control. Fusion 44 (2002) R27</ref>.  


LRC in floating potential fluctuations has been investigated in the proximity of the density-limit in the NBI plasma scenarios in TJ-II [Fig. 2]. The density limit decreases with the magnetic field (B = 0.7 – 1 T) in qualitative agreement with the empirical stellarator scaling law for density limit [5]. At low densities the LRCs, measured at rho ≈ 0.9 for frequencies below 20 kHz, are quite large (≈ 0.8) and vary only slightly with increasing density. When approaching the density-limit the amplitude of LRC reduces rapidly with increasing plasma density, in agreement with previous results <ref>Y. Xu et al  Nucl. Fusion 51 (2011) 063020</ref>. The reduction in the LRC as approaching the density limit is accompanied by a reduction in edge mean radial electric field and the level of plasma turbulence.  Results point to the role of collisionality, mean E × B flows and level of turbulence on the amplitude of zonal flows in the proximity of the density limit.  
LRC in floating potential fluctuations has been investigated in the proximity of the density-limit in the NBI plasma scenarios in TJ-II. The density limit decreases with the magnetic field (B = 0.7 – 1 T) in qualitative agreement with the empirical stellarator scaling law for density limit [5]. At low densities the LRCs, measured at rho ≈ 0.9 for frequencies below 20 kHz, are quite large (≈ 0.8) and vary only slightly with increasing density. When approaching the density-limit the amplitude of LRC reduces rapidly with increasing plasma density, in agreement with previous results <ref>Y. Xu et al  Nucl. Fusion 51 (2011) 063020</ref>. The reduction in the LRC as approaching the density limit is accompanied by a reduction in edge mean radial electric field and the level of plasma turbulence.  Results point to the role of collisionality, mean E × B flows and level of turbulence on the amplitude of zonal flows in the proximity of the density limit.  
TJ-II findings suggest that at a threshold radiation value for the density limit the degradation of confinement would be partially due to the damping of Zonal Flows as recently pointed out <ref>R. J. Hajjar et al., Physics of Plasmas 25 (2018) 062306</ref>. If this is the case, density limit in stellarators would depend on the transport optimization criteria, a prediction that could be validated experimentally.  
TJ-II findings suggest that at a threshold radiation value for the density limit the degradation of confinement would be partially due to the damping of Zonal Flows as recently pointed out <ref>R. J. Hajjar et al., Physics of Plasmas 25 (2018) 062306</ref>. If this is the case, density limit in stellarators would depend on the transport optimization criteria, a prediction that could be validated experimentally.


== International or National funding project or entity ==
== International or National funding project or entity ==
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