dc.contributor.author | Cortázar, O. D. | |
dc.contributor.author | Megía-Macías, A. | |
dc.contributor.author | Vizcaíno-de-Julián, A. | |
dc.contributor.author | Tarvainen, Olli | |
dc.contributor.author | Komppula, Jani | |
dc.contributor.author | Koivisto, Hannu | |
dc.date.accessioned | 2016-01-21T12:11:16Z | |
dc.date.available | 2016-01-21T12:11:16Z | |
dc.date.issued | 2014 | |
dc.identifier.citation | Cortázar, 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.other | CONVID_23704252 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/48412 | |
dc.description.abstract | First 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.iso | eng | |
dc.publisher | American Institute of Physics | |
dc.relation.ispartofseries | Review of Scientific Instruments | |
dc.subject.other | frame images | |
dc.subject.other | magnetic field configuration | |
dc.subject.other | microwave power | |
dc.subject.other | gas pressure | |
dc.title | Ultra-fast intensified frame images from an electron cyclotron resonance hydrogen plasma at 2.45 GHz: Some space distributions of visible and monochromatic emissions | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-201601211220 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.contributor.oppiaine | Fysiikka | fi |
dc.contributor.oppiaine | Kiihdytinlaboratorio | fi |
dc.contributor.oppiaine | Physics | en |
dc.contributor.oppiaine | Accelerator Laboratory | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.date.updated | 2016-01-21T07:15:05Z | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 0034-6748 | |
dc.relation.numberinseries | 2 | |
dc.relation.volume | 85 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © 2013 AIP Publishing LLC. Published in this repository with the kind permission of the publisher. | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.relation.doi | 10.1063/1.4824812 | |
dc.type.okm | A1 | |