Spatial and Temporal Structure of Edge-Localized Modes

A. Kirk, H. R. Wilson, G. F. Counsell, R. Akers, E. Arends, S. C. Cowley, J. Dowling, B. Lloyd, M. Price, and M. Walsh (MAST Team)
Phys. Rev. Lett. 92, 245002 – Published 16 June 2004

Abstract

This Letter provides information on the spatial and temporal structure of periodic eruptions observed in magnetically confined laboratory fusion plasmas, called edge-localized modes (ELMs), and highlights similarities with solar eruptions. Taken together, the observations presented in this Letter provide strong evidence for ELMs being associated with a filamentlike structure. These filaments are extended along a field line, are generated on a 100   μs time scale, erupt from the outboard side, and connect back into the plasma. Such structures are predicted by a theoretical model based on the “ballooning” instability, developed for both solar and tokamak applications.

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  • Received 21 January 2004

DOI:https://doi.org/10.1103/PhysRevLett.92.245002

©2004 American Physical Society

Authors & Affiliations

A. Kirk1, H. R. Wilson1, G. F. Counsell1, R. Akers1, E. Arends1,2, S. C. Cowley1,3, J. Dowling1, B. Lloyd1, M. Price1, and M. Walsh1,4 (MAST Team1)

  • 1EURATOM/UKAEA Fusion Association, Culham Science Centre, Abingdon, Oxon OX14 3DB, United Kingdom
  • 2FOM-Institute for Plasma Physics “Rijnhuizen”, Edisonbaan 14, NL-3439 MN Nieuwegein, The Netherlands
  • 3Imperial College of Science and Technology, University of London, London SW7 2BZ, United Kingdom, and Department of Physics and Astronomy, UCLA, Los Angeles, California 90095, USA
  • 4Walsh Scientific Ltd., Culham Science Centre, Abingdon, Oxon OX14 3EB, United Kingdom

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Issue

Vol. 92, Iss. 24 — 18 June 2004

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