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Observation of energetic electron confinement in a largely stochastic reversed-field pinch plasma

  • D. J. Clayton
  • , B. E. Chapman
  • , R. O'Connell
  • , A. F. Almagri
  • , D. R. Burke
  • , C. B. Forest
  • , J. A. Goetz
  • , M. C. Kaufman
  • , F. Bonomo
  • , P. Franz
  • , M. Gobbin
  • , P. Piovesan

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

Runaway electrons with energies >100 keV are observed with the appearance of an m=1 magnetic island in the core of otherwise stochastic Madison Symmetric Torus [Dexter, Fusion Technol. 19, 131 (1991)] reversed-field-pinch plasmas. The island is associated with the innermost resonant tearing mode, which is usually the largest in the m=1 spectrum. The island appears over a range of mode spectra, from those with a weakly dominant mode to those, referred to as quasi single helicity, with a strongly dominant mode. In a stochastic field, the rate of electron loss increases with electron parallel velocity. Hence, high-energy electrons imply a region of reduced stochasticity. The global energy confinement time is about the same as in plasmas without high-energy electrons or an island in the core. Hence, the region of reduced stochasticity must be localized. Within a numerical reconstruction of the magnetic field topology, high-energy electrons are substantially better confined inside the island, relative to the external region. Therefore, it is deduced that the island provides a region of reduced stochasticity and that the high-energy electrons are generated and well confined within this region.

Original languageEnglish
Article number012505
JournalPhysics of Plasmas
Volume17
Issue number1
DOIs
StatePublished - 2010
Externally publishedYes

Funding

The authors would like to thank the MST team for their support in this research and the RFX-mod team for their collaboration. This work was supported by the U.S. Department of Energy cooperative agreement DE-FC02-05ER54814.

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