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dc.contributor.authorGeorge, Anand
dc.contributor.authorKalvas, Taneli
dc.contributor.authorMelanson, Stephane
dc.contributor.authorSavard, Nicolas
dc.contributor.authorPotkins, Dave
dc.contributor.authorDehnel, Morgan
dc.contributor.authorBroderick, Neil G. R.
dc.date.accessioned2020-01-21T12:05:32Z
dc.date.available2020-01-21T12:05:32Z
dc.date.issued2020
dc.identifier.citationGeorge, A., Kalvas, T., Melanson, S., Savard, N., Potkins, D., Dehnel, M., & Broderick, N. G. R. (2020). A study of the optical effect of plasma sheath in a negative ion source using IBSIMU code. <i>Review of Scientific Instruments</i>, <i>91</i>(1), Article 013306. <a href="https://doi.org/10.1063/1.5129603" target="_blank">https://doi.org/10.1063/1.5129603</a>
dc.identifier.otherCONVID_34147382
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/67425
dc.description.abstractA plasma sheath inside an ion source has a strong focusing effect on the formation of an ion beam from the plasma. Properties of the beam depend on the shape and location of the plasma sheath inside the source. The most accessible experimental data dependent on the plasma sheath are the beam phase space distribution. Variation of beam emittance is a reflection of the properties of the plasma sheath, with minimum emittance for the optimal shape of the plasma sheath. The location and shape of the plasma sheath are governed by complex physics and can be understood by simulations using plasma models in particle tracking codes like IBSimu. In the current study, a model of the D-Pace’s TRIUMF licensed filament powered volume-cusp negative ion source is made using the IBSimu code. Beam emittance trends are compared between experiments and simulations.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Institute of Physics
dc.relation.ispartofseriesReview of Scientific Instruments
dc.rightsIn Copyright
dc.subject.otherplasma sheath
dc.subject.othernegative ion source
dc.titleA study of the optical effect of plasma sheath in a negative ion source using IBSIMU code
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-202001211378
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.issn0034-6748
dc.relation.numberinseries1
dc.relation.volume91
dc.type.versionpublishedVersion
dc.rights.copyright© 2020 AIP Publishing
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.subject.ysoplasmafysiikka
dc.subject.ysohiukkaskiihdyttimet
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p10238
jyx.subject.urihttp://www.yso.fi/onto/yso/p14309
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1063/1.5129603
dc.type.okmA1


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