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Zolotarev, K.

Paper Title Page
WEPE092 Mechanical and Vacuum Design of the Wiggler Section of the ILC Damping Rings 3563
 
  • O.B. Malyshev
    STFC/DL/ASTeC, Daresbury, Warrington, Cheshire
  • N.A. Collomb, J.M. Lucas, S. Postlethwaite
    STFC/DL, Daresbury, Warrington, Cheshire
  • M. Korostelev
    The University of Liverpool, Liverpool
  • A. Wolski
    Cockcroft Institute, Warrington, Cheshire
  • K. Zolotarev
    BINP SB RAS, Novosibirsk
 
 

A vacuum vessel design of wiggler sections should meet a few challenging specification. The SR power of about 40 kW is generated in each wiggler. Expanding fan of SR radiation reaches the beam vacuum chamber walls in the following wiggler and may cause the following problem: massive power dissipation on vacuum chamber walls inside the cryogenic vessel, radiation damage of superconducting coil, high photo-electron production rate that cause an e-cloud build-up to unacceptable level. Therefore this power should be absorbed in the places where these effects are tolerable or manageable. A few possible solutions for tackling all SR related problems as well as vacuum design are discussed in the paper in details.

 
WEPE094 SR Power Distribution along Wiggler Section of ILC DR 3569
 
  • O.B. Malyshev
    STFC/DL/ASTeC, Daresbury, Warrington, Cheshire
  • N.A. Collomb, J.M. Lucas, S. Postlethwaite
    STFC/DL, Daresbury, Warrington, Cheshire
  • M. Korostelev
    The University of Liverpool, Liverpool
  • A. Wolski
    Cockcroft Institute, Warrington, Cheshire
  • K. Zolotarev
    BINP SB RAS, Novosibirsk
 
 

A 374-m long wiggler section is a key part of ILC damping ring that should alloy reaching a low beam emittance for the ILC experiment. Synchrotron radiation generated by the beam in the wigglers should be absorbed by different components of vacuum vessel, including specially designed absorbers. The optimisation of the mechanical design, vacuum system and anti-e-cloud mitigation requires accurate calculation of the SR power distribution. The angular power distribution from a single wiggler was calculated with in-house developed software. Then the superposition of SR from all wigglers allows calculating power distribution for all components along the wiggler section and the downstream straight section.

 
WEPE089 Design Optimisation for the CLIC Damping Rings 3554
 
  • Y. Papaphilippou, F. Antoniou, M.J. Barnes, S. Bettoni, S. Calatroni, P. Chiggiato, R. Corsini, A. Grudiev, R. Maccaferri, M. Modena, L. Rinolfi, G. Rumolo, D. Schoerling, D. Schulte, M. Taborelli, A. Vivoli
    CERN, Geneva
  • E.B. Levichev, S.V. Sinyatkin, P. Vobly, K. Zolotarev
    BINP SB RAS, Novosibirsk
 
 

The CLIC damping rings should produce the ultra-low emittance necessary for the high luminosity performance of the collider. This combined to the high bunch charge present a number of beam dynamics and technical challenges for the rings. Lattice studies have been focused on low emittance cells with optics that reduce the effect Intra-beam scattering. The final beam emittance is reached with the help of super-conducting damping wigglers. Results from recent simulations and prototype measurements are presented, including a detailed absorption scheme design. Collective effects such as electron cloud and fast ion instability can severely limit the performance and mitigation techniques have been identified and tested. Tolerances for alignment and technical system design such as kickers, RF cavities, magnets and vacuum have been finally established.