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dc.contributor.authorCortázar, O. D.
dc.contributor.authorMegía-Macías, A.
dc.contributor.authorVizcaíno-de-Julián, A.
dc.contributor.authorTarvainen, Olli
dc.contributor.authorKomppula, Jani
dc.contributor.authorKoivisto, Hannu
dc.date.accessioned2016-01-21T12:11:16Z
dc.date.available2016-01-21T12:11:16Z
dc.date.issued2014
dc.identifier.citationCortázar, O. D., Megía-Macías, A., Vizcaíno-de-Julián, A., Tarvainen, O., Komppula, J., & Koivisto, H. (2014). Ultra-fast intensified frame images from an electron cyclotron resonance hydrogen plasma at 2.45 GHz: Some space distributions of visible and monochromatic emissions. <i>Review of Scientific Instruments</i>, <i>85</i>(2), Article 02A902. <a href="https://doi.org/10.1063/1.4824812" target="_blank">https://doi.org/10.1063/1.4824812</a>
dc.identifier.otherCONVID_23704252
dc.identifier.otherTUTKAID_62029
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/48412
dc.description.abstractFirst results from an ultra-fast frame image acquisition diagnostic coupled to a 2.45 GHz microwave hydrogen discharge are presented. The plasma reactor has been modified to include a transparent doubled shielded quartz window allowing to viewing the full plasma volume. Pictures describing the breakdown process at 1μs exposure time have been obtained for integrated visible light signal, Balmer-alpha, Balmer-beta lines, and Fulcher-band. Several different plasma emission distributions are reported. The distribution depends on the magnetic field configuration, incident microwave power, and neutral gas pressure.
dc.language.isoeng
dc.publisherAmerican Institute of Physics
dc.relation.ispartofseriesReview of Scientific Instruments
dc.subject.otherframe images
dc.subject.othermagnetic field configuration
dc.subject.othermicrowave power
dc.subject.othergas pressure
dc.titleUltra-fast intensified frame images from an electron cyclotron resonance hydrogen plasma at 2.45 GHz: Some space distributions of visible and monochromatic emissions
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201601211220
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiaineKiihdytinlaboratoriofi
dc.contributor.oppiainePhysicsen
dc.contributor.oppiaineAccelerator Laboratoryen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2016-01-21T07:15:05Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn0034-6748
dc.relation.numberinseries2
dc.relation.volume85
dc.type.versionpublishedVersion
dc.rights.copyright© 2013 AIP Publishing LLC. Published in this repository with the kind permission of the publisher.
dc.rights.accesslevelopenAccessfi
dc.relation.doi10.1063/1.4824812
dc.type.okmA1


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