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dc.contributor.authorBhaskar, B. S.
dc.contributor.authorKoivisto, H.
dc.contributor.authorTarvainen, O.
dc.contributor.authorThuillier, T.
dc.contributor.authorToivanen, V.
dc.date.accessioned2022-02-01T05:50:18Z
dc.date.available2022-02-01T05:50:18Z
dc.date.issued2022
dc.identifier.citationBhaskar, B. S., Koivisto, H., Tarvainen, O., Thuillier, T., & Toivanen, V. (2022). Quasi-periodical kinetic instabilities in minimum-B confined plasma. <i>AIP Advances</i>, <i>12</i>(1), Article 015223. <a href="https://doi.org/10.1063/5.0070824" target="_blank">https://doi.org/10.1063/5.0070824</a>
dc.identifier.otherCONVID_104066400
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/79589
dc.description.abstractWe 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.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAIP Publishing
dc.relation.ispartofseriesAIP Advances
dc.rightsCC BY 4.0
dc.subject.otherECR-ionilähteet
dc.subject.otherplasma confinement
dc.subject.otherplasma heating
dc.subject.otherplasma instabilities
dc.subject.othercyclotron resonance
dc.subject.otherion sources
dc.titleQuasi-periodical kinetic instabilities in minimum-B confined plasma
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-202202011352
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2158-3226
dc.relation.numberinseries1
dc.relation.volume12
dc.type.versionpublishedVersion
dc.rights.copyright© 2022 Author(s).
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.relation.grantnumber315855
dc.subject.ysosyklotronit
dc.subject.ysoplasmafysiikka
dc.subject.ysohiukkaskiihdyttimet
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15295
jyx.subject.urihttp://www.yso.fi/onto/yso/p10238
jyx.subject.urihttp://www.yso.fi/onto/yso/p14309
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1063/5.0070824
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundinginformationThis work was supported by the Academy of Finland Project funding (Grant No. 315855) and the University of Grenoble Alpes under the EMERGENCE program.
datacite.isSupplementedBy.doi10.23729/4a5436c7-c428-49e9-81c8-b242a5bf7e80
datacite.isSupplementedBySubhash Bhasi Bhaskar, Bichu; Toivanen, Ville; Koivisto, Hannu; Tarvainen, Olli; Thuillier, Thomas. (2023). <i>JYFL-ACCLAB-ISG004 Study of the temporal structure of kinetic instabilities in ECR-heated plasma</i>. University of Jyväskylä. <a href="https://doi.org/10.23729/4a5436c7-c428-49e9-81c8-b242a5bf7e80" target="_blank">https://doi.org/10.23729/4a5436c7-c428-49e9-81c8-b242a5bf7e80</a>.
dc.type.okmA1


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