Quasi-periodical kinetic instabilities in minimum-B confined plasma

Abstract
We present the results of an experimental investigation of quasi-periodical kinetic instabilities exhibited by magnetically confined electron cyclotron resonance heated plasmas. The instabilities were detected by measuring plasma microwave emission, electron losses, and wall bremsstrahlung. The instabilities were found to be grouped into fast sequences of periodic plasma losses, separated by ∼100 µs between the bursts, followed by 1–10 ms quiescent periods before the next event. Increasing the plasma energy content by adjusting the plasma heating parameters, in particular the magnetic field strength, makes the instabilities more chaotic in the time domain. Statistical analysis reveals that the energy released in a single instability event depends on the magnetic field strength and microwave power but not on the neutral gas pressure. The effects of these ion source parameters on the instability characteristics are explained qualitatively by considering their influence on the electron energy distribution. A correlation is found between the energy dissipated in an instability event and the recovery time of the periodic bursts, i.e., a large amplitude instability leads to a long recovery time of the electron energy distribution.
Main Authors
Format
Articles Research article
Published
2022
Series
Subjects
Publication in research information system
Publisher
AIP Publishing
The permanent address of the publication
https://urn.fi/URN:NBN:fi:jyu-202202011352Use this for linking
Review status
Peer reviewed
ISSN
2158-3226
DOI
https://doi.org/10.1063/5.0070824
Language
English
Published in
AIP Advances
Citation
  • Bhaskar, B. S., Koivisto, H., Tarvainen, O., Thuillier, T., & Toivanen, V. (2022). Quasi-periodical kinetic instabilities in minimum-B confined plasma. AIP Advances, 12(1), Article 015223. https://doi.org/10.1063/5.0070824
License
CC BY 4.0Open Access
Funder(s)
Research Council of Finland
Funding program(s)
Academy Project, AoF
Akatemiahanke, SA
Research Council of Finland
Additional information about funding
This work was supported by the Academy of Finland Project funding (Grant No. 315855) and the University of Grenoble Alpes under the EMERGENCE program.
Copyright© 2022 Author(s).

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