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Status of new 18 GHz ECRIS HIISI

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.
Main Authors
Kalvas, Taneli Koivisto, Hannu Tarvainen, Olli Lettry, Jacques Mahner, Edgar Marsh, Bruce Pardo, Richard Scrivens, Richard
Format
Conferences Conference paper
Published
2018
Series
AIP Conference Proceedings
Subjects
heavy ion ion source injector
HIISI
accelerator laboratory
University of Jyväskylä
ionit
säteilyfysiikka
syklotronit
tutkimuslaitteet
Publication in research information system
https://converis.jyu.fi/converis/portal/detail/Publication/28651320
Publisher
AIP Publishing
The permanent address of the publication
https://urn.fi/URN:NBN:fi:jyu-201810084378Käytä tätä linkitykseen.
Parent publication ISBN
978-0-7354-1727-4
Review status
Peer reviewed
ISSN
0094-243X
DOI
https://doi.org/10.1063/1.5053280
Conference
International Conference on Ion Sources
Language
English
Published in
AIP Conference Proceedings
Is part of publication
Proceedings of the 17th International Conference on Ion Sources
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.), Proceedings of the 17th International Conference on Ion Sources (Article 040006). AIP Publishing. AIP Conference Proceedings, 2011. https://doi.org/10.1063/1.5053280
License
In CopyrightOpen Access
Funder(s)
European Commission
Funding program(s)
Research infrastructures, H2020
Research infrastructures, H2020
European Commission
Additional information about funding
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.
Copyright© AIP Publishing, 2018

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