dc.contributor.author | Kalvas, Taneli | |
dc.contributor.author | Koivisto, Hannu | |
dc.contributor.author | Tarvainen, Olli | |
dc.contributor.editor | Lettry, Jacques | |
dc.contributor.editor | Mahner, Edgar | |
dc.contributor.editor | Marsh, Bruce | |
dc.contributor.editor | Pardo, Richard | |
dc.contributor.editor | Scrivens, Richard | |
dc.date.accessioned | 2018-10-29T06:11:33Z | |
dc.date.available | 2019-09-22T21:35:23Z | |
dc.date.issued | 2018 | |
dc.identifier.citation | Kalvas, T., Koivisto, H., & Tarvainen, O. (2018). Status of new 18 GHz ECRIS HIISI. In J. Lettry, E. Mahner, B. Marsh, R. Pardo, & R. Scrivens (Eds.), <i>Proceedings of the 17th International Conference on Ion Sources</i> (Article 040006). AIP Publishing. AIP Conference Proceedings, 2011. <a href="https://doi.org/10.1063/1.5053280" target="_blank">https://doi.org/10.1063/1.5053280</a> | |
dc.identifier.other | CONVID_28651320 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/59974 | |
dc.description.abstract | A new 18 GHz ECR ion source HIISI is under commissioning at the Accelerator Laboratory at the University of Jyväskylä (JYFL). The main purpose of HIISI is to produce high-energy beam cocktails, e.g. Xe44+, for radiation effects testing of electronics with the K130 cyclotron. The initial commissioning results in 18+14 GHz operation with oxygen, argon and xenon are reported. The beam currents are compared to those produced by reference ion sources (JYFL 14 GHz ECRIS, GTS and SuSI). At the moment (October 2017) 560 µA of O6+ and 310 µA of Ar13+, for example, have been reached with HIISI at 2.3 kW total power. | fi |
dc.format.mimetype | application/pdf | |
dc.language.iso | eng | |
dc.publisher | AIP Publishing | |
dc.relation.ispartof | Proceedings of the 17th International Conference on Ion Sources | |
dc.relation.ispartofseries | AIP Conference Proceedings | |
dc.rights | In Copyright | |
dc.subject.other | heavy ion ion source injector | |
dc.subject.other | HIISI | |
dc.subject.other | accelerator laboratory | |
dc.subject.other | University of Jyväskylä | |
dc.title | Status of new 18 GHz ECRIS HIISI | |
dc.type | conference paper | |
dc.identifier.urn | URN:NBN:fi:jyu-201810084378 | |
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/ConferencePaper | |
dc.date.updated | 2018-10-08T09:15:22Z | |
dc.relation.isbn | 978-0-7354-1727-4 | |
dc.type.coar | http://purl.org/coar/resource_type/c_5794 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 0094-243X | |
dc.relation.numberinseries | 2011 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | © AIP Publishing, 2018 | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | conferenceObject | |
dc.relation.conference | International Conference on Ion Sources | |
dc.relation.grantnumber | 654002 | |
dc.relation.grantnumber | 654002 | |
dc.relation.projectid | info:eu-repo/grantAgreement/EC/H2020/654002/EU// | |
dc.subject.yso | ionit | |
dc.subject.yso | säteilyfysiikka | |
dc.subject.yso | syklotronit | |
dc.subject.yso | tutkimuslaitteet | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p9015 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p11069 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15295 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p2440 | |
dc.rights.url | http://rightsstatements.org/page/InC/1.0/?language=en | |
dc.relation.doi | 10.1063/1.5053280 | |
dc.relation.funder | Euroopan komissio | fi |
dc.relation.funder | European Commission | en |
jyx.fundingprogram | Research infrastructures, H2020 | fi |
jyx.fundingprogram | Research infrastructures, H2020 | en |
jyx.fundinginformation | The project has received funding from the European Unions Horizon 2020 research and innovation programme under
grant agreement No 654002, from the Academy of Finland under the Finnish Centre of Excellence Programme 2012–
2017 (Nuclear and Accelerator Based Physics Research at JYFL) and under FIRI grant agreement No 273526. This
work has been funded also by the European Space Research and Technology Centre, European Space Agency, under ESA/GSTP ESTEC/Contract No. 4000112736/14/NL/PA. | |
dc.type.okm | A4 | |