The Proposed Conversion of CESR to an ILC Damping Ring Test Facility

Slides:



Advertisements
Similar presentations
ILC Damping Ring R&D Using CESR Mark Palmer Cornell Laboratory for Accelerator-Based Science and Education.
Advertisements

CESR as Light Source David L. Rubin for the CESR Operations Group Cornell University Laboratory for Elementary-Particle Physics.
SuperB Damping Rings M. Biagini, LNF-INFN P. Raimondi, SLAC/INFN A. Wolski, Cockroft Institute, UK SuperB III Workshop, SLAC, June 2006.
SuperB and the ILC Damping Rings Andy Wolski University of Liverpool/Cockcroft Institute 27 April, 2006.
CESR-c Status CESR Layout - Pretzel, Wigglers, solenoid compensation Performance to date Design parameters Our understanding of shortfall Plans for remediation.
Overview of ILC Plans D.Rubin April 17, D. Rubin2 ILC R&D Activities and Plans 1.Positron Source 2.Damping Ring 3.Low Emittance Transport - damping.
Low Emittance Program David Rubin Cornell Laboratory for Accelerator-Based Sciences and Education CesrTA.
Experimental Plan for Achieving Low Emittance in CesrTA David Rubin Cornell Laboratory for Accelerator-Based Sciences and Education.
Low Emittance Program David Rubin Cornell Laboratory for Accelerator-Based Sciences and Education CesrTA.
July 22, 2005Modeling1 Modeling CESR-c D. Rubin. July 22, 2005Modeling2 Simulation Comparison of simulation results with measurements Simulated Dependence.
Ultra-Low Emittance Storage Ring David L. Rubin December 22, 2011.
March 7, 2007 LET Issues (Cai/Kubo/Zisman) Global Design Effort 1 Low-Emittance Tuning Issues and Plans Yunhai Cai, Kiyoshi Kubo and Michael S. Zisman.
January 13, 2004D. Rubin - Cornell1 CESR-c BESIII/CLEO-c Workshop, IHEP January 13, 2004 D.Rubin for the CESR operations group.
Y. Ohnishi / KEK KEKB-LER for ILC Damping Ring Study Simulation of low emittance lattice includes machine errors and optics corrections. Y. Ohnishi / KEK.
Y. Ohnishi / KEK KEKB LER for ILC Damping Ring Study Lattice simulation of lattice errors and optics corrections. November 1, 2007 Y. Ohnishi / KEK.
Project Management Mark Palmer Cornell Laboratory for Accelerator-Based Sciences and Education.
CASA Collider Design Review Retreat HERA The Only Lepton-Hadron Collider Ever Been Built Worldwide Yuhong Zhang February 24, 2010.
CesrTA Experimental Plan M. Palmer for the CesrTA Collaboration November 17, 2008.
Emittance Measurement Needs for CesrTF M. Palmer Cornell University Laboratory for Elementary-Particle Physics.
CesrTA Status Report & R&D Planning Mark Palmer Cornell University April 21, 2010.
November 14, 2004First ILC Workshop1 CESR-c Wiggler Dynamics D.Rubin -Objectives -Specifications -Modeling and simulation -Machine measurements/ analysis.
1 Proposal for a CESR Damping Ring Test Facility M. Palmer & D.Rubin November 8, 2005.
July 16-17, 2007 Joint NSF/DOE Review of CesrTA Proposal 1 * Mitigation techniques planning still underway with ILC DR group Answer to Questions 1 and.
Vertical Emittance Tuning at the Australian Synchrotron Light Source Rohan Dowd Presented by Eugene Tan.
1 Alternative ILC Bunch Compressor 7 th Nov KNU (Kyungpook National Univ.) Eun-San Kim.
1 Alternative Bunch Compressor 30 th Sep KNU Eun-San Kim.
02/04/2009 AS-TAGL Mtg Global Design Effort 1 CesrTA Update Mark Palmer CLASSE.
Motivation and Overview David Rubin Cornell Laboratory for Accelerator-Based Sciences and Education.
The SPS as a Damping Ring Test Facility for CLIC March 6 th, 2013 Yannis PAPAPHILIPPOU CERN CLIC Collaboration Working meeting.
Kiyoshi Kubo Electron beam in undulators of e+ source - Emittance and orbit angle with quad misalignment and corrections - Effect of beam pipe.
February 5, 2005D. Rubin - Cornell1 CESR-c Status -Operations/Luminosity -Machine studies -Simulation and modeling -4.1GeV.
The Introduction to CSNS Accelerators Oct. 5, 2010 Sheng Wang AP group, Accelerator Centre,IHEP, CAS.
ATF status M. Ross October 15, 2004 The ATF is the largest test facility built exclusively for linear collider RD –Utility not reduced by the selection.
Summary David Rubin Cornell Laboratory for Accelerator-Based Sciences and Education.
ILC Damping Ring R&D Using CESR Mark Palmer Cornell Laboratory for Accelerator-Based Science and Education.
CESR Test Accelerator Optics Correction and Tuning Tools David Sagan Cornell University.
Global Design Effort ILC Damping Rings: R&D Plan and Organisation in the Technical Design Phase Andy Wolski University of Liverpool and the Cockcroft Institute,
CESR as Light Source David Rubin for the CESR Operations Group Cornell University Laboratory for Elementary-Particle Physics.
ILC Damping Rings: Configuration Status and R&D Plans Andy Wolski Lawrence Berkeley National Laboratory January 19, 2006.
Characterization of the Fast Ion Instability at CesrTA David Rubin Cornell University.
V.Shiltsev 1 Comments on What Kind of Test Facility(ies) the ILC Needs Vladimir Shiltsev/ Fermilab.
CESR-c Plans for CESR (or Life Without CLEO) Mark A. Palmer David L. Rubin Second ILC Accelerator Workshop August 18, 2005.
1 DR 10 Hz Repetition Rate S. Guiducci (LNF) AD&I webex, 23 June 2010.
Simulation for Lower emittance in ATF Damping Ring Kiyoshi Kubo Similar talk in DR WS in Frascati, May 2007 Most simulations were done several.
Arun Saini, N. Solyak Fermi National Accelerator Laboratory
ILC DR Lower Horizontal Emittance, preliminary study
J. Alexander + Cornell accelerator group Cornell University
For Discussion Possible Beam Dynamics Issues in ILC downstream of Damping Ring LCWS2015 K. Kubo.
ILC Z-pole Calibration Runs Main Linac performance
CesrTA Status Report Mark Palmer July 8, 2009.
ILC DR Lower Horizontal Emittance? -2
CesrTA Status and Planning
Coupling Correction at the Australian Synchrotron
Electron Cloud Studies at CESR-c and CesrTA
IntraBeam Scattering Calculation
sx* Limitations and Improvements Paths
Recent Electron Cloud Studies at CESR and Future Plans
Low Emittance Tuning in CESR TA
Progress activities in short bunch compressors
M. Tigner, R. Helms, M. Palmer, D. Rubin, D. Sagan Cornell University
Low Emittance Tuning David Rubin Cornell Laboratory for
CesrTA Experimental Schedule and Priorities
Status of Low Emittance Tuning at CESR TA
CLIC damping rings working plan towards the CDR
CesrTA Low Emittance Program David Rubin Cornell Laboratory for
Proposal for a CESR Damping Ring Test Facility
Sawtooth effect in CEPC PDR/APDR
Yuri Nosochkov Yunhai Cai, Fanglei Lin, Vasiliy Morozov
Fanglei Lin JLEIC R&D Meeting, August 4, 2016
DYNAMIC APERTURE OF JLEIC ELECTRON COLLIDER
Presentation transcript:

The Proposed Conversion of CESR to an ILC Damping Ring Test Facility M. Palmer, R. Helms, D. Rubin, D. Sagan, J. Urban, M. Ehrlichman Abstract: In 2008 the Cornell Electron Storage Ring (CESR) will end nearly three decades of providing electron-positron collisions for the CLEO experiment. At that time it will be possible to reconfigure CESR as a damping ring test facility, CesrTF, for the International Linear Collider project. With its 12 damping wigglers, CesrTF will offer horizontal emittance in the few nanometer range and, ideally, vertical emittances approaching those specified for the ILC damping rings. An important feature of the CesrTF concept is the ability to operate with positrons or electrons. Positron operation will allow detailed testing of electron cloud issues critical for the operation of the ILC positron damping rings. Other key features include operation with wigglers that meet or exceed all ILC damping ring requirements, the ability to operate from 1.5 to 5.5 GeV beam energies, and the provision of a large insertion region for testing damping ring hardware. We discuss the CesrTF machine parameters, critical conversion issues, and experimental reach for damping ring studies. CesrTF Baseline Lattice CesrTF Conversion Dynamic Aperture bx North IR with Wigglers (Top View) Lattice design carried out with 6 wigglers in North IR and 6 wigglers in the CESR arcs. Zero dispersion regions created for all wigglers. by ~18 m Frequency Map Analysis Color Scale: Points plotted at ½ damping time Tunes calculated for 1st half and 2nd half of damping time South IR with RF Cavities for Short Bunch Operation (Top View) Wiggler Locations hx Move 6 wigglers to North IR Add cryogenic support Add electron cloud diagnostics Space for insertion devices in South IR Ample cryogenics support SCRF cavities for short bunch length operation Instrumentation (eg, possible laserwire installation) Could support an extraction line Upgrade feedback system for 4 ns spaced bunches Upgrade beam instrumentation Ultra-low emittance measurement CLEO North IR South IR 14W 15W 14E 15E 19E 19W Wiggler Moves Target ey~ 5 – 10 pm Parameter Value E 2.0 GeV Nwiggler 12 Bmax 2.1 T ex 2.25 nm Qx 14.59 Qy 9.63 Qz 0.098 sE/E 8.6 x 10-4 tx,y 47 ms sz 6.8 mm ap 6.4 x 10-3 Tune Scans to Determine Working Point Intrabeam Scattering (Preliminary) Low Emittance Operation Nominal CESR Magnet Alignment Resolutions Equilibrium Emittance with IBS for Baseline Lattice Calculation assumes vertical emittance is dominantly due to emittance coupling. ex grows by factor of ~3 from zero current to ILC bunch current Nominal Values Misalignment Nominal Value Quadrupole, Bend and Wiggler Offsets 150 mm Sextupole Offsets 300 mm Quadrupole, Bend, Wiggler and Sextupole Rotations 100 mrad Example Vertical Emittance Sensitivities IBS growth rates scale as 1/g4 a increase energy Increases zero current emittance Decreases sensitivity to IBS Can also lengthen bunch Explore 2.5 GeV lattice with 9 mm bunch as potential configuration for low emittance studies at the ILC bunch current (eg, electron cloud studies) Dominant Sensitivity Correction Algorithm Randomly misalign elements using multiple seeds Orbit correction followed by dispersion correction using steering and skew quadrupole correctors Include effects of BPM errors Equilibrium Emittance for 2.5 GeV Lattice and 9mm Bunch Length ex grows by a factor of < 1.6 from zero current to ILC bunch current. Zero current ex ~2.85 nm. . Correction Type Average Value 95% Limit Orbit Only 10.2 pm 21.4 pm Orbit+Dispersion 3.9 pm 8.2 pm CESR-c/CLEO-c program ends on March 31, 2008 7-9 month conversion followed by commissioning Available for ILC DR R&D in early 2009 Operating Schedule Approximately 110 running days/year in 2 periods Interleaved with CHESS X-ray running Significant downtime at each transition for installation of prototypes and other hardware Minimum of 3 years of operation as a test facility Conclusion: Simulations indicate that CesrTF can be operated in a regime that is useful for a range of damping ring studies. In particular, CesrTF will have the ability to study physics issues associated with the damping ring wigglers and validate the final design of the ILC wigglers and vacuum chamber. The machine will be able to directly explore the impact of the electron cloud on the emittance. Due to the modest scope of the conversion, CesrTF offers an efficient route towards exploring key areas of ILC damping ring physics and technology on a timescale consistent with the start of ILC construction. Conversion and Operations Plan