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Crittenden, J.A.

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MO4PBC03 Developments for Cornell's X-Ray ERL 106
 
  • J.A. Crittenden, I.V. Bazarov, S.A. Belomestnykh, D.H. Bilderback, M.G. Billing, J.D. Brock, E.P. Chojnacki, B.M. Dunham, M. P. Ehrlichman, M.J. Forster, S.M. Gruner, G.H. Hoffstaetter, Y. Li, M. Liepe, C.E. Mayes, A.A. Mikhailichenko, H. Padamsee, S.B. Peck, D. Sagan, V.D. Shemelin, A.B. Temnykh, M. Tigner, V. Veshcherevich
    CLASSE, Ithaca, New York
  • C. Johnstone
    Fermilab, Batavia
 
 

Cornell University is planning to build an Energy-Recovery Linac (ERL) X-ray facility. In this ERL design, a 5 GeV superconducting linear accelerator extends the CESR ring which is currently used for the Cornell High Energy Synchrotron Source (CHESS). Here we describe some of the recent developments for this ERL, including linear and nonlinear optics, tracking studies, vacuum system design, gas and intra beam scattering computations, and collimator and radiation shielding calculations based on this optics, undulator developments, optimization of X-ray beams by electron beam manipulation, technical design of ERL cavities and cryomodules, and preparation of the accelerator site.

 

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TH5PFP047 Electron Cloud Modeling Considerations at CesrTA 3306
 
  • J.R. Calvey, J.A. Crittenden, G. Dugan, M.A. Palmer
    CLASSE, Ithaca, New York
  • C.M. Celata
    LBNL, Berkeley, California
 
 

Funding: Support provided by the US National Science Foundation and the US Department of Energy


The Cornell Electron Storage Ring (CESR) has recently begun operation as a test accelerator for next generation linear collider damping rings. This program, known as CesrTA, includes a thorough investigation of synchrotron radiation generated electron cloud effects. CESR is capable of operating with a variety of bunch patterns and beam currents, as well as with both electron and positron beams. Understanding the buildup of the cloud under these conditions requires the use of well validated simulation programs. This paper will discuss three such programs- POSINST, ECLOUD and CLOUDLAND, which have been benchmarked against each other in parameter regimes relevant to CesrTA operating conditions, with the aim of understanding systematic differences in the calculations.

 
FR5RFP043 Simulations of Electron-Cloud Current Density Measurements in Dipoles, Drifts and Wigglers at CesrTA 4628
 
  • J.R. Calvey, J.A. Crittenden, G. Dugan, S. Greenwald, D.L. Kreinick, J.A. Livezey, M.A. Palmer, D. L. Rubin
    CLASSE, Ithaca, New York
  • C.M. Celata, M.A. Furman, G. Penn, M. Venturini
    LBNL, Berkeley, California
  • K.C. Harkay
    ANL, Argonne
  • P. Jain, K. Kanazawa, Y. Suetsugu
    KEK, Ibaraki
  • M.T.F. Pivi, L. Wang
    SLAC, Menlo Park, California
 
 

Funding: Supported by the US National Science Foundation, the US Department of Energy under Contracts No. DE-AC02-06CH11357, DE-AC02-05CH11231, and DE-AC02-76SF00515, and by the Japan/US Cooperation Program.


CESR at Cornell has been operating as a damping ring test accelerator (CesrTA) with beam parameters approaching those anticipated for the ILC damping rings. A core component of the research program is to fully understand electron cloud effects in CesrTA. As a local probe of the electron cloud, several segmented retarding field analyzers (RFAs) have been installed in CesrTA in dipole, drift and wiggler regions. Using these RFAs, the energy spectrum of the time-average electron cloud current density striking the walls has been measured for a variety of bunch train patterns; with bunch populations up to 2x1010 per bunch, beam energies from 2 to 5 GeV, horizontal geometric emittances from roughly 10 to 133 nm, and bunch lengths of about 1 cm; and for both positron and electron beams. The effect of mitigation measures, such as coatings, has also been studied. This paper will compare these measurements with the predictions of simulation programs, and discuss the implications of these comparisons for our understanding of the physics of electron cloud generation and mitigation in ILC-like damping rings.

 
FR5RFP044 Studies of the Effects of Electron Cloud Formation on Beam Dynamics at CesrTA 4631
 
  • J.A. Crittenden, J.R. Calvey, G. Dugan, D.L. Kreinick, J.A. Livezey, M.A. Palmer, D. L. Rubin
    CLASSE, Ithaca, New York
  • M.A. Furman, G. Penn, M. Venturini
    LBNL, Berkeley, California
  • K.C. Harkay
    ANL, Argonne
  • R. Holtzapple
    CalPoly, San Luis Obispo, CA
  • K. Ohmi
    KEK, Ibaraki
  • M.T.F. Pivi, L. Wang
    SLAC, Menlo Park, California
 
 

Funding: National Science Foundation award 0734867 Office of Science, U.S. Department of Energy contracts DE-AC02-05CH11231 and DE-AC02-06CH11357


The Cornell Electron Storage Ring Test Accelerator (CesrTA) has commenced operation as a linear collider damping ring test bed following its conversion from an e+e- collider in 2008. A core component of the research program is the measurement of effects of synchrotron-radiation-induced electron cloud formation on beam dynamics. We have studied the interaction of the beam with the cloud in a number of experiments, including measurements of coherent tune shifts and emittance growth in various bunch train configurations, with different bunch currents, beam energies, beam emittance, and bunch lengths, for both positron and electron beams. This paper compares these measurements to modeling results from several advanced cloud simulation algorithms and discusses the implications of these comparisons for our understanding of the physics of electron cloud formation and decay in damping rings of the type proposed for future high-energy linear colliders.

 
FR1RAI02 The Conversion and Operation of the Cornell Electron Storage Ring as a Test Accelerator (CesrTA) for Damping Rings Research and Development 4200
 
  • M.A. Palmer, J.P. Alexander, M.G. Billing, J.R. Calvey, S.S. Chapman, G.W. Codner, C.J. Conolly, J.A. Crittenden, J. Dobbins, G. Dugan, E. Fontes, M.J. Forster, R.E. Gallagher, S.W. Gray, S. Greenwald, D.L. Hartill, W.H. Hopkins, J. Kandaswamy, D.L. Kreinick, Y. Li, X. Liu, J.A. Livezey, A. Lyndaker, V. Medjidzade, R.E. Meller, S.B. Peck, D.P. Peterson, M.C. Rendina, P. Revesz, D.H. Rice, N.T. Rider, D. L. Rubin, D. Sagan, J.J. Savino, R.D. Seeley, J.W. Sexton, J.P. Shanks, J.P. Sikora, K.W. Smolenski, C.R. Strohman, A.B. Temnykh, M. Tigner, S. Vishniakou, W.S. Whitney, T. Wilksen, H.A. Williams
    CLASSE, Ithaca, New York
  • J.M. Byrd, C.M. Celata, J.N. Corlett, S. De Santis, M.A. Furman, A. Jackson, R. Kraft, D.V. Munson, G. Penn, D.W. Plate, A.W. Rawlins, M. Venturini, M.S. Zisman
    LBNL, Berkeley, California
  • J.W. Flanagan, P. Jain, K. Kanazawa, K. Ohmi, H. Sakai, K. Shibata, Y. Suetsugu
    KEK, Ibaraki
  • K.C. Harkay
    ANL, Argonne
  • Y. He, M.C. Ross, C.-Y. Tan, R.M. Zwaska
    Fermilab, Batavia
  • R. Holtzapple
    CalPoly, San Luis Obispo, CA
  • J.K. Jones
    STFC/DL/ASTeC, Daresbury, Warrington, Cheshire
  • D. Kharakh, M.T.F. Pivi, L. Wang
    SLAC, Menlo Park, California
  • E.N. Smith
    Cornell University, Ithaca, New York
  • A. Wolski
    Cockcroft Institute, Warrington, Cheshire
 
 

Funding: Support provided by the US National Science Foundation, the US Department of Energy, and the Japan/US Cooperation Program.


In March of 2008, the Cornell Electron Storage Ring (CESR) concluded twenty eight years of colliding beam operations for the CLEO high energy physics experiment. We have reconfigured CESR as an ultra low emittance damping ring for use as a test accelerator (CesrTA) for International Linear Collider (ILC) damping ring R&D. The primary goals of the CesrTA program are to achieve a beam emittance approaching that of the ILC Damping Rings with a positron beam, to investigate the interaction of the electron cloud with both low emittance positron and electron beams, to explore methods to suppress the electron cloud, and to develop suitable advanced instrumentation required for these experimental studies (in particular a fast x-ray beam size monitor capable of single pass measurements of individual bunches). We report on progress with the CESR conversion activities, the status and schedule for the experimental program, and the first experimental results that have been obtained.

 

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