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ELMs and fast edge fluctuations in Alcator C-Mod

  • J. A. Snipes
  • , R. S. Granetz
  • , M. Greenwald
  • , A. E. Hubbard
  • , I. H. Hutchinson
  • , J. Irby
  • , J. Kesner
  • , S. Migliuolo
  • , T. Sunn Pedersen
  • , J. Ramos
  • , J. Rice
  • , P. C. Stek
  • , Y. Takase
  • , S. M. Wolfe

Research output: Contribution to journalArticlepeer-review

Abstract

Just above the H-mode threshold power at low density, small amplitude high repetition rate (1-5 kHz) type III edge-localized modes (ELMs) are observed. At higher input power, the H-modes become ELM-free. At high density and high input power (n̄e > 2.2 × 1020 m-3, Pin > 2 MW), the plasma often enters a new H-mode regime now called the enhanced Dα H-mode, which is a steady-state H-mode often without distinct ELMs but with high levels of Dα emission. Enhanced Dα H-modes are accompanied by persistent high-frequency broadband (50-400 kHz) density and magnetic fluctuations. Above about n̄e > 3 × 1020 m-3, the enhanced Dα H-modes may also exhibit bursting or continuous low m, n coherent magnetic fluctuations with frequencies from 60-90 kHz. In the H-mode, steep edge gradients are observed with a nine-channel electron cyclotron emission (ECE) polychromator and a 38-channel, high-resolution, edge soft-x-ray array. The soft-x-ray pedestal width remains around 3 to 4 mm in the ELM-free H-mode and between type III ELMs. The pedestal collapses within 100 μs during an ELM. Calculations indicate that the plasma in the H-mode is often near ideal ballooning first stability limits, but no type I ELMs have yet been identified. Edge micro-tearing modes destabilized by a steep temperature gradient are also considered as a possible explanation of the observed fluctuations during the enhanced Dα H-mode.

Original languageEnglish (US)
Pages (from-to)765-770
Number of pages6
JournalPlasma Physics and Controlled Fusion
Volume40
Issue number5
DOIs
StatePublished - 1998
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Nuclear Energy and Engineering
  • Condensed Matter Physics

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