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Title: Progress of superconducting electron cyclotron resonance ion sources at Institute of Modern Physics (IMP)

Journal Article · · Review of Scientific Instruments
DOI:https://doi.org/10.1063/1.4825164· OSTI ID:22253687
; ; ; ; ; ; ; ; ;  [1];  [1];  [2];  [3]
  1. Institute of Modern Physics, CAS, Lanzhou 730000 (China)
  2. University of Chinese Academy of Sciences, Beijing 100049 (China)
  3. Nuclear Science Division, LBNL, Berkeley, California 94720 (United States)

Superconducting ECR ion sources can produce intense highly charged ion beams for the application in heavy ion accelerators. Superconducting Electron Resonance ion source with Advanced Design (SECRAL) is one of the few fully superconducting ECR ion sources that has been successfully built and put into routine operation for years. With enormous efforts and R and D work, promising results have been achieved with the ion source. Heated by the microwave power from a 7 kW/24 GHz gyrotron microwave generator, very intense highly charged gaseous ion beams have been produced, such as 455 eμA Xe{sup 27+}, 236 eμA Xe{sup 30+}, and 64 eμA Xe{sup 35+}. Since heavy metallic ion beams are being more and more attractive and important for many accelerator projects globally, intensive studies have been made to produce highly charged heavy metal ion beams, such as those from bismuth and uranium. Recently, 420 eμA Bi{sup 30+} and 202 eμA U{sup 33+} have been produced with SECRAL source. This paper will present the latest results with SECRAL, and the operation status will be discussed as well. An introduction of recently started SECRAL II project will also be given in the presentation.

OSTI ID:
22253687
Journal Information:
Review of Scientific Instruments, Vol. 85, Issue 2; Conference: ICIS 2011: 14. international conference on ion sources, Giardini-Naxos, Sicily (Italy), 12-16 Sep 2011; Other Information: (c) 2013 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 0034-6748
Country of Publication:
United States
Language:
English

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