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dc.contributor.authorToivanen, V.
dc.contributor.authorBhaskar, B. S.
dc.contributor.authorKoivisto, H.
dc.contributor.authorMaunoury, L.
dc.contributor.authorTarvainen, O.
dc.contributor.authorThuillier, T.
dc.date.accessioned2022-01-18T13:34:53Z
dc.date.available2022-01-18T13:34:53Z
dc.date.issued2022
dc.identifier.citationToivanen, V., Bhaskar, B. S., Koivisto, H., Maunoury, L., Tarvainen, O., & Thuillier, T. (2022). Influence of axial mirror ratios on the kinetic instability threshold in electron cyclotron resonance ion source plasma. <i>Physics of Plasmas</i>, <i>29</i>(1), Article 013501. <a href="https://doi.org/10.1063/5.0069638" target="_blank">https://doi.org/10.1063/5.0069638</a>
dc.identifier.otherCONVID_103853872
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/79401
dc.description.abstractElectron Cyclotron Resonance (ECR) ion source plasmas are prone to kinetic instabilities. The onset of the instabilities manifests as emission of microwaves, bursts of electrons expelled from the plasma volume, and the collapse of the extracted highly charged ion (HCI) currents. Consequently, the instabilities limit the HCI performance of ECR ion sources by limiting the parameter space available for ion source optimization. Previous studies have shown that the transition from stable to unstable plasma regime is strongly influenced by the magnetic field structure, especially the minimum field value inside the magnetic trap (Bmin). This work focuses to study the role of the magnetic confinement on the onset of the kinetic instabilities by probing the influence of the injection and extraction mirror field variation on the instability threshold. The experiments have been performed with a room-temperature 14.5 GHz ECR ion source with an axially movable middle coil that provides flexible control over the axial field profile and especially the Bmin, which was used to quantify the variation in the instability threshold. The experimental results show that variation of the extraction field Bext, which defines the weakest magnetic mirror, correlates systematically with the variation of the instability threshold; decreasing the Bext allows higher threshold Bmin. The result demonstrates the importance of electron confinement and losses on the plasma stability. The connection between the weakest mirror field and the onset of instabilities is discussed taking into account the variation of magnetic field gradient and resonance plasma volume.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Institute of Physics
dc.relation.ispartofseriesPhysics of Plasmas
dc.rightsIn Copyright
dc.subject.otherplasma confinement
dc.subject.otherelectron energy distribution functions
dc.subject.otherplasma heating
dc.subject.othermagnetic mirrors
dc.subject.othercyclotron resonance
dc.subject.otherions and properties
dc.subject.otherplasma instabilities
dc.subject.otherion sources
dc.titleInfluence of axial mirror ratios on the kinetic instability threshold in electron cyclotron resonance ion source plasma
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202201181170
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn1070-664X
dc.relation.numberinseries1
dc.relation.volume29
dc.type.versionpublishedVersion
dc.rights.copyright© 2022 the Authors
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber315855
dc.subject.ysoplasmafysiikka
dc.subject.ysosyklotronit
dc.subject.ysohiukkaskiihdyttimet
dc.subject.ysoplasma (kaasut)
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p10238
jyx.subject.urihttp://www.yso.fi/onto/yso/p15295
jyx.subject.urihttp://www.yso.fi/onto/yso/p14309
jyx.subject.urihttp://www.yso.fi/onto/yso/p238
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1063/5.0069638
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundinginformationThis work has been supported by the Academy of Finland Project funding (No. 315855) and University of Grenoble Alpes under the EMERGENCE program.
dc.type.okmA1


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