Keyword: heavy-ion
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TUA2WD03 Automated Operation of EBIS Injector at BNL target, operation, linac, laser 153
 
  • T. Kanesue, E.N. Beebe, S. Binello, B.D. Coe, M.R. Costanzo, L. DeSanto, S. Ikeda, J.P. Jamilkowski, N.A. Kling, D. Lehn, C.J. Liaw, V. Lo Destro, D.R. McCafferty, J. Morris, M. Okamura, R.H. Olsen, D. Raparia, R. Schoepfer, F. Severino, L. Smart, K. Zeno
    BNL, Upton, Long Island, New York, USA
 
  The RHIC-EBIS pre-injector is a heavy ion pre-injector to deliver multiple heavy ion species at 2 MeV/u to the AGS-Booster at the RHIC accelerator complex. In addition to collider experiments at RHIC, multiple heavy ion species are used for the NASA Space Radiation Laboratory (NSRL) to evaluate the risk of radiation in space in radiobiology, physics, and engineering. A GCR simulator is one of the operation modes of NSRL to simulate a galactic cosmic ray event, which requires switching multiple ion species within a short period of time. The RHIC-EBIS pre-injector delivers various heavy ion species independently for simultaneous operation of RHIC and NSRL. We developed an automated scheme of the rapid species change and it is routinely used by NSRL or Main Control Room for daily operation without assistance of RHIC-EBIS experts. The number of species change exceeds one hundred. This paper describes the automated operation of the RHIC-EBIS pre-injector and the operational performance.
This work has been supported by Brookhaven Science Associates, LLC under Contract No. DE-SC0012704 with the U.S. Department of Energy, and by the National Aeronautics and Space Administration.
 
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DOI • reference for this paper ※ https://doi.org/10.18429/JACoW-HB2018-TUA2WD03  
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WEP1WB03 First Heavy Ion Beam Acceleration with a Superconducting Multi Gap CH-cavity cavity, linac, acceleration, emittance 215
 
  • W.A. Barth, M. Heilmann, A. Rubin, A. Schnase, S. Yaramyshev
    GSI, Darmstadt, Germany
  • K. Aulenbacher, W.A. Barth, F.D. Dziuba, V. Gettmann, T. Kürzeder, M. Miski-Oglu
    HIM, Mainz, Germany
  • K. Aulenbacher
    IKP, Mainz, Germany
  • M. Basten, M. Busch, H. Podlech, M. Schwarz
    IAP, Frankfurt am Main, Germany
 
  A newly developed superconducting 15-gap RF-cavity has been successfully tested at GSI Helmholtzzentrum für Schwerionenforschung. After a short commissioning and ramp up time of some days, a Crossbar H-cavity accelerated first time heavy ion beams with full transmission up to the design beam energy of 1.85 MeV/u. The design acceleration gain of 3.5 MV inside a length of less than 70 cm has been verified with heavy ion beam of up to 1.5 particle mueA. The measured beam parameters showed excellent beam quality, while a dedicated beam dynamics layout provides beam energy variation between 1.2 and 2.2 MeV/u. The beam commissioning is a milestone of the R&D work of Helmholtz Institute Mainz and GSI in collaboration with Goethe University Frankfurt towards a superconducting heavy ion continuous wave linear accelerator cw-Linac with variable beam energy. Further linac beam dynamics layout issues will be presented as well.  
slides icon Slides WEP1WB03 [20.157 MB]  
DOI • reference for this paper ※ https://doi.org/10.18429/JACoW-HB2018-WEP1WB03  
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THP2WC03 The Choosing of Magnetic Structure of Isochronous Cyclotron DC-130 for Applied Research cyclotron, operation, acceleration, extraction 446
 
  • I.A. Ivanenko, J. Franko, G.G. Gulbekyan, I.V. Kalagin, N.Yu. Kazarinov
    JINR, Dubna, Moscow Region, Russia
 
  At the present time, the activities on creation of the new multipurpose isochronous cyclotron DC130 are carried out at the FLNR, JINR. The cyclotron DC130 is intended for microchip testing, production of track pore membranes and for applied physics. The cyclotron will accelerate the heavy ions with mass-to-charge ratio A/Z from 5 to 8 up to the fixed energies 2 and 4.5 MeV per nucleon. The main magnet and acceleration system of DC130 is based on the U200 cyclotron that now is under reconstruction. At the present paper the method of choosing of main magnet parameters of cyclotron is described.  
DOI • reference for this paper ※ https://doi.org/10.18429/JACoW-HB2018-THP2WC03  
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