Author: Safranek, J.A.
Paper Title Page
TUPHA012 LOCO Application to NSLS2 SR Dispersion and Beta Beating Correction 1989
 
  • X. Yang
    BNL, Upton, Long Island, New York, USA
  • X. Huang, J.A. Safranek
    SLAC, Menlo Park, California, USA
 
  During the short run in early July, 2014, we made changes to the Matlab LOCO setup for NSLS-II and applied LOCO successfully to the machine. The MML setup was verified with I/O tests for all quadrupole families. The LOCO setup was further tested with an intentional quadrupole error. After the successful LOCO correction, the rms beta beat was reduced from the initial values of 5.5% x and 5.6% y, to 1.9% x and 1.0% y, respectively. The rms horizontal dispersion error was reduced from 21 mm to 6 mm. It is critical to keep the same closed orbit for LOCO correction to take effect. Because presently some correctors are nearly saturated, closed orbit cannot be controlled for additional iterations. We expect LOCO to achieve better optics correction after the orbit control is improved.  
DOI • reference for this paper ※ https://doi.org/10.18429/JACoW-IPAC2015-TUPHA012  
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WEBD2 Survey of Commissioning of Recent Storage Ring Light Sources 2482
 
  • M. Borland
    ANL, Argonne, Ilinois, USA
  • R. Bartolini, I.P.S. Martin
    DLS, Oxfordshire, United Kingdom
  • L.O. Dallin
    CLS, Saskatoon, Saskatchewan, Canada
  • P. Kuske, R. Müller
    HZB, Berlin, Germany
  • L.S. Nadolski
    SOLEIL, Gif-sur-Yvette, France
  • F. Pérez
    ALBA-CELLS Synchrotron, Cerdanyola del Vallès, Spain
  • J.A. Safranek
    SLAC, Menlo Park, California, USA
  • S. Shin
    PAL, Pohang, Kyungbuk, Republic of Korea
  • Z.T. Zhentang
    SINAP, Shanghai, People's Republic of China
 
  Funding: Work supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357.
The Advanced Photon Source and other existing storage ring light sources are contemplating replacing an existing, operating storage ring with a multi-bend achromat lattice. One issue is that existing light sources have large user communities who are greatly inconvenienced by extended shutdowns. Hence, there will be a premium placed on rapid commissioning of the new lattice. To better understand the possibilities, we undertook a survey of recent commissioning experience at third-generation light sources. We present a summary of that survey here.
 
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DOI • reference for this paper ※ https://doi.org/10.18429/JACoW-IPAC2015-WEBD2  
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