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Spatio-temporal evolution of the H → L back transition

  • Author(s): Miki, K
  • Diamond, PH
  • Schmitz, L
  • McDonald, DC
  • Estrada, T
  • Gürcan, OD
  • Tynan, GR
  • et al.

Published Web Location

https://doi.org/10.1063/1.4812555Creative Commons 'BY-NC-ND' version 4.0 license
Abstract

Since ITER will operate close to threshold and with limited control, the H → L back transition is a topic important for machine operations as well as physics. Using a reduced mesoscale model [Miki, Phys. Plasmas 19, 092306 (2012)], we investigate ELM-free H → L back transition dynamics in order to isolate transport physics effects. Model studies indicate that turbulence spreading is the key process which triggers the back transition. The transition involves a feedback loop linking turbulence and profiles. The I-phase appears during the back transition following a slow power ramp down, while fast ramp-downs reveal a single burst of zonal flow during the back transition. The I-phase nucleates at the pedestal shoulder, as this is the site of the residual turbulence in H-mode. Hysteresis in the profile gradient scale length is characterized by the Nusselt number, where Nu = χi, turb/χi, neo. Relative hysteresis of temperature gradient vs density gradient is sensitive to the pedestal Prandtl number, where Pr ped = D ped/χ i, neo. We expect the H-mode to be somewhat more resilient in density than in temperature. © 2013 AIP Publishing LLC.

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