CesrTA Electron Cloud R&D Overview Mark Palmer Cornell Laboratory for Accelerator-Based Sciences and Education.

Slides:



Advertisements
Similar presentations
Electron-cloud instability in the CLIC damping ring for positrons H. Bartosik, G. Iadarola, Y. Papaphilippou, G. Rumolo TWIICE workshop, TWIICE.
Advertisements

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.
ECLOUD Calculations of Coherent Tune Shifts for the April 2007 Measurements - Study of SEY Model Effects - Jim Crittenden Cornell Laboratory for Accelerator-Based.
Global design effort 2008 DOE/NSF review June 30, 2008 Global design effort Americas Slide 1 CesrTA Status and Planning for FY08-09 David Rubin Mark Palmer.
Damping Rings Baseline Lattice Choice ILC DR Technical Baseline Review Frascati, July 7, 2011 Mark Palmer Cornell University.
LEPP, the Cornell University Laboratory for Elementary-Particle Physics, has joined with CHESS to become the Cornell Laboratory for Accelerator-based Sciences.
45 th ICFA Beam Dynamic Workshop June 8–12, 2009, Cornell University, Ithaca New York Recent Studies with ECLOUD Jim Crittenden Cornell Laboratory for.
ElectronsdFud Simulation Work at Cornell Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education.
CESR Beam-Beam Effects at CESR Mark A. Palmer Cornell University July 14, 2001.
ECLOUD Simulations for CESR Witness Bunch Tune Shift Measurements Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education.
Electron Cloud Simulation Work at Cornell Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education.
2011 Damping Rings Lattice Evaluation Mark Palmer Cornell University March 8, 2011.
Ultra-Low Emittance Storage Ring David L. Rubin December 22, 2011.
25-26 June, 2009 CesrTA Workshop CTA09 Electron Cloud Single-Bunch Instability Modeling using CMAD M. Pivi CesrTA CTA09 Workshop June 2009.
August 9, 2007M. Palmer1 CESR Machine Studies Planning Overview Principal Projects Other Milestones and Dates Machine Studies Schedule Proposed Plan.
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.
Recent electron cloud studies at CESR David Rice Cornell University Laboratory for Elementary-Particle Physics.
Beam dynamics on damping rings and beam-beam interaction Dec 포항 가속기 연구소 김 은 산.
Project Management Mark Palmer Cornell Laboratory for Accelerator-Based Sciences and Education.
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.
Electron cloud in the wigglers of ILC Damping Rings L. Wang SLAC ILC Damping Rings R&D Workshop - ILCDR06 September 26-28, 2006 Cornell University.
CesrTA EC Build-Up and Mitigation Program - Introduction Mark Palmer June 25, 2009.
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.
October 13,2010 WG Meeting Cornell U. Recommendation for Electron Cloud Mitigations in the ILC Damping Ring ILC DR Working Group October 13, 2010 Cornell.
Electron Cloud Mitigation Studies at CesrTA Joseph Calvey 10/1/2009.
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.
C ESR TA Status Report July 22, 2010 Mark Palmer for the C ESR TA Collaboration.
Cesr-TA Simulations: Overview and Status G. Dugan, Cornell University LCWS-08.
Electron cloud measurements and simulations at CesrTA G. Dugan, Cornell University 4/19/09 TILC09 4/18/09.
Highlights from the ILCDR08 Workshop (Cornell, 8-11 July 2008) report by S. Calatroni and G. Rumolo, in CLIC Meeting Goals of the workshop:
CesrTA Vacuum System Conversion and Operational Experiences Yulin Li for the CesrTA Team Cornell Laboratory for Accelerator-based ScienceS and Education.
CesrTA Status Report Mark Palmer Cornell University September 2, 2009.
01/08/2009 AS-TAGL Mtg Global Design Effort 1 CesrTA Update Mark Palmer CLASSE.
February 5, 2005D. Rubin - Cornell1 CESR-c Status -Operations/Luminosity -Machine studies -Simulation and modeling -4.1GeV.
Summary David Rubin Cornell Laboratory for Accelerator-Based Sciences and Education.
CESR Test Accelerator Optics Correction and Tuning Tools David Sagan Cornell University.
WebEx meeting November 17, 2009 ILC Damping Ring Working Group on Electron Cloud LC e- cloud Working Group November 17, 2009.
XBSM Analysis - Dan Peterson Review of the optics elements: Pinhole (“GAP”), FZP, Coded Aperture Extracting information from the GAP what is the GAP width?
LEPP, the Cornell University Laboratory for Elementary-Particle Physics, has joined with CHESS to become the Cornell Laboratory for Accelerator-based Sciences.
ILC Damping Ring Test Facilities Status Report Mark Palmer Cornell University May 9, 2009 ILC PAC Review, Vancouver.
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,
3 February 2010 ILC Damping Ring electron cloud WG effort Mauro Pivi SLAC on behalf of ILC DR working group on e- cloud ILC DR Webex Meeting Jan 3, 2010.
Characterization of the Fast Ion Instability at CesrTA David Rubin Cornell University.
CESR-c Plans for CESR (or Life Without CLEO) Mark A. Palmer David L. Rubin Second ILC Accelerator Workshop August 18, 2005.
Electron Cloud Experimental Plans at Cesr-TA ILCDR08 - July 10, 2009 G. Dugan Cornell Laboratory for Accelerator-Based Sciences and Education.
49th ICFA Advanced Beam Dynamics Workshop. October 8–12, 2010 LEPP, the Cornell University Laboratory for Elementary-Particle Physics, has joined with.
Mark Palmer for the CESRTA Collaboration
Electron Cloud and Ion Experimental Program
Electron Cloud R&D at Cornell ILCDR08--7/8/08
CesrTA Status Report Mark Palmer July 8, 2009.
CesrTA Status and Planning
Detailed Characterization of Vacuum Chamber Surface Properties Using Measurements of the Time Dependence of Electron Cloud Development Jim Crittenden.
RECENT DEVELOPMENTS IN MODELING
Why Study Electron Clouds? Methods and Tools to Study Electron Clouds
J.A.Crittenden, Y.Li, X.Liu, M.A.Palmer, J.P.Sikora (Cornell)
Recent Electron Cloud Studies at CESR and Future Plans
CESRTA Measurement of Electron Cloud Density by TE Wave and RFA
M. Tigner, R. Helms, M. Palmer, D. Rubin, D. Sagan Cornell University
The Proposed Conversion of CESR to an ILC Damping Ring Test Facility
CesrTA Experimental Schedule and Priorities
Electron cloud studies at CESR
CesrTA Wiggler RFA Measurements
CTA 09 - Introduction David Rubin Cornell Laboratory for
Proposal for a CESR Damping Ring Test Facility
Presentation transcript:

CesrTA Electron Cloud R&D Overview Mark Palmer Cornell Laboratory for Accelerator-Based Sciences and Education

2March 5, 2008 TILC08 - Sendai, Japan Experimental Goals & Techniques –Electron Cloud Growth Studies –Beam Dynamics Studies –Measurement techniques studied to date Engineering Preparations Collaboration Outline

3March 5, 2008 TILC08 - Sendai, Japan CesrTA Goals I Electron Cloud Growth Studies –Provide a “laboratory” for the study of EC growth Particularly in regions of greatest concern for DR : wigglers and dipoles Provide suitable diagnostics to characterize the growth in all key regions –Characterize the performance of mitigation techniques in dipoles, quadrupoles and wigglers –Explore a parameter regime that approximates the ILC DR Bunch train configuration –Bunch charge, length, spacing, emittance –Inter-train gaps Energy Investigate parameter dependence  Detailed data with which to benchmark ILC simulations  Demonstrate suitable vacuum chamber technologies

4March 5, 2008 TILC08 - Sendai, Japan CesrTA Goals II Electron Cloud Induced Instability and Emittance Dilution –Characterize the impact of the cloud on witness bunches/trains trailing an initial EC-generating train Provide sufficient local diagnostics to characterize EC growth and decay in all representative chambers Control EC density and distribution around ring by witness bunch delay and/or intensity of generating train Explore a range of witness bunch parameters (emittance, charge, energy etc) Species-dependent studies in same chamber –Distinguish impedance effects  Detailed data with which to benchmark ILC simulations

5March 5, 2008 TILC08 - Sendai, Japan CesrTA EC Program Summary CesrTA will provide: –Detailed local EC growth measurements with which to benchmark the relevant simulation codes –Detailed studies of EC mitigation in critical vacuum chambers –Beam dynamics measurements over significant parameter ranges to verify key inputs to the instability modeling codes and to benchmark their performance The goal of our program is to demonstrate key EC mitigation technologies, measure instabilities and emittance growth, and validate EC simulations in a regime approaching that of the ILC DR on a timescale consistent with the EDR.

6March 5, 2008 TILC08 - Sendai, Japan EC Growth Studies Install chambers with EC growth diagnostics and mitigation –Goal is to have implemented diagnostics in each representative chamber type by mid-2009 Heavy reliance on segmented Retarding Field Analyzers –Wiggler chambers in L0 straight w/mitigation –Dipole chambers in arcs w/mitigation –Quadrupole chambers w/mitigation L0 and L3 straights –Drifts Diagnostics adjacent to test chambers Solenoids –Some components to be provided by collaborators L3 RFA Test Chamber

7March 5, 2008 TILC08 - Sendai, Japan Components of the EC Growth Plan L3 Straight –Instrument large bore quadrupoles and adjacent drifts –Proposed location for diagnostic chicane Arcs where wigglers removed –Instrumented dipoles and adjacent drifts L0 Straight –Instrumented wiggler straight and adjacent sections Pressure bump capability planned for major diagnostic regions –Impact on ECE (and FII?)

8March 5, 2008 TILC08 - Sendai, Japan Beam Dynamics Studies Prerequisites –Instrumentation to characterize bunch trains at ultra low emittance Multibunch detectors and readouts High resolution beam profile monitor –Ring operation at ultra low emittance Instability Studies –Focus on witness bunch studies where EC density controlled by intensity of leading train and delay to witness bunches –Detailed study of instability thresholds and emittance growth versus the witness bunch-train parameters –Detailed electron-positron comparisons to help distinguish the dynamics and to evaluate EC impact on the electron beam –Have de-scoped plans to study fast ion effects for the electron beam as part of this program Measurements of instabilities and emittance growth along electron bunch trains Explore the dependence on emittance, bunch charge and spacing, train gaps and vacuum pressure

9March 5, 2008 TILC08 - Sendai, Japan Witness Bunch Studies – e + Vertical Tune Shift Initial train of 10 bunches  generate EC Measure tune shift and beamsize for witness bunches at various spacings Bunch-by-bunch, turn-by-turn beam position monitor 1 kHz    e ~ 1.5 x m -3 Ohmi, etal, APAC01, p.445 Positron Beam, 0.75 mA/bunch, 14 ns spacing, 1.9 GeV Operation Preliminary Error bars represent scatter observed during a sequence of measurements

10March 5, 2008 TILC08 - Sendai, Japan Data and Simulation Initial comparisons for CESR –Growth modeling for dipole chambers –Initial level of agreement is promising Ongoing Effort –Model full ring and explore parameter space –Limited MS opportunities during final CLEO-c run ECLOUD Program SEY = 1.4 Dipole Region Preliminary Overlay simulated EC density on vertical tune shift data Soft value – trade off Between  max and E peak

11March 5, 2008 TILC08 - Sendai, Japan Witness Bunch Studies – e - Vertical Tune Shift Same setup as for positrons Negative vertical tune shift and long decay consistent with EC –Implications for the electron DR? Electron Beam, 0.75 mA/bunch, 14 ns spacing, 1.9 GeV Operation Preliminary Results Negative vertical tune shift along train  consistent with EC Magnitude of shift along train is ~1/4 th of shift for positron beam NOTE: Shift continues to grow for 1 st 4 witness bunches!

12March 5, 2008 TILC08 - Sendai, Japan EC Induced Instability Vertical beam size along 45 bunch e+ trains (2 GeV, 14 ns bunch spacing) –Range of bunch currents – turn averages collected for each point Observe onset of instability moving forward in train with increasing bunch current – consistent with EC

13March 5, 2008 TILC08 - Sendai, Japan Present Focus – Engineering Prep During final CLEO-c production run –Limited machine studies time –Main focus on engineering preparations for CesrTA downs in May and July Key pieces for EC program –L0 wiggler experimental area –EC diagnostics Retarding Field Analysers Suitable readout electronics –Vacuum chamber designs –Instrumentation preparation

14March 5, 2008 TILC08 - Sendai, Japan MAIN COMPONENT POSITIONS L0 Wiggler Region L0 wiggler experimental region design work well underway –Installation during July down –Heavily instrumented throughout with vacuum diagnostics –Targeting full design review this month followed by full scale production Note: Part of CLEO will remain in place –At present unable to remove full detector –Time savings

15March 5, 2008 TILC08 - Sendai, Japan Retarding Field Analysers Beam tests have continued through CLEO-c conclusion Upgraded readout electronics for large channel count RFAs are now ready for production Thin RFA structure performing well Positron beam shadowed at test location

16March 5, 2008 TILC08 - Sendai, Japan RFA Wiggler VC Delivered Chambers with Thin RFAs Loss of US collaborators impacted development heavily –Cornell has picked up detailed design –Now ready for final design review –Working with KEK to see whether construction support might be available

17March 5, 2008 TILC08 - Sendai, Japan CesrTA Vacuum Chambers CesrTA Wiggler Modifications Remove Cu beam-pipe Replace with beam-pipe having EC suppression and diagnostics CESR-c Wiggler Chambers Vertical beam stay-clear: 50mm ILC DR assumes 46mm dia. pipe

18March 5, 2008 TILC08 - Sendai, Japan CESR Dipole Chamber RFA RFA on Dipole VC Prototyping Underway

March 5, 2008TILC08 - Sendai, JapanJim Alexander19 X-Ray Beam Size Monitor for CESRTA Bunch-by-bunch measurements of beam profile for fast emittance determination Image individual bunches spaced by 4ns. Transverse resolution << 10~15  m beam size Non-destructive measurement. Flexible operation. Start simple, allow various upgrade paths.

March 5, 2008TILC08 - Sendai, JapanJim Alexander20 Features that affect performance Detector: Pixel size Absorption Carrier mobility pq Monochromator: Surface quality - flatness  Bandwidth  Reflectivity Source: Diffraction from source of known angular divergence Bunch current, critical energy, etc  D N Zone Plate: Diffraction - finite D Chromatic aberration Transparency Optical path: Magnification Backgrounds Vacuum window: Absorption Uniformity Readout: Equivalent noise charge Bandwidth Color coding: Photon yield Resolution Distortions Speed

March 5, 2008TILC08 - Sendai, JapanJim Alexander21 Interrelationships and Optimization Fresnel Criterion Diffraction limited resolution (SR fan) Image-object-focal length relation Magnification of one-lens system 7 Equations in 9 unknowns. optimize over remaining variables: source- lens distance (p), and x-ray wavelength (. Match bandwidth of monochromator Objective lens encompasses all of SR fan Set magnification for optimal sampling in pixel detector

March 5, 2008TILC08 - Sendai, JapanJim Alexander22 Parameters for CESRTA xray Beam Size Monitor

March 5, 2008TILC08 - Sendai, JapanJim Alexander23 Sidebar: Resolution, Precision, and Photon Statistics Optical transfer function is characterized by a resolution (point spread function). This is a fixed property of the optical system. For CESRTA design, it is 2-3  m. (Figure at right assumes 3.5  m) Photon statistics (and electronic noise, if applicable) fluctuate from snapshot to snapshot. The measurement precision of this system is determined by the stochastic element, not the fixed correction*. (m)(m) * Residual uncertainty in the optical resolution will appear as a systematic error Resolution Stochastic band (photon statistics) 800 photons 400 photons True Value Measured Value Precision

March 5, 2008TILC08 - Sendai, JapanJim Alexander24 Sensors GaAs/InGaAs 1-dim photodiode array –512 diodes, 25  m x 500  m –Hamamatsu G D –Off-the-shelf Why GaAs? –High carrier mobility (8400 cm 2 /Vs) & drift velocity (200  m/ns) –High Z, high density short abs length ~ 1  m at 2.5keV –Room temperature ops. –Good radiation hardness –Commodity parts available; IR receivers for 10Gbps optical ethernet Fast: << 1ns

March 5, 2008TILC08 - Sendai, JapanJim Alexander25 Single GaAs photodiode (46  m dia) Optics: pinhole. (40  m vertical slit) White beam (no monochromator) Data acquisition: 72MHz (14ns interval); 12 bit ADC. Mechanically scanned vertically and horizontally through the beam -- “synthetic aperture camera” Single bunch, single pass data - no averaging over turns. Prototype study, in CHESS (Slide 1) Pinhole (40  m vertical slit) Detector 10.5m 2.9m Beam  y ~ 140  m Hard bend magnet,  = 31m Beam energy 5.3 GeV 45 bunches, 150~200mA Bunch charge 6~8x10 10 Mechanical stage Horizontal slit (1 mm)

March 5, 2008TILC08 - Sendai, JapanJim Alexander26 Result of vertical beam scan (single pixel) Measured: S/N e = 27 photons per bunch is ~400 Signal risetime << 300ps Observed beam size 142  9  m (expect ~150) Calculated: Energy abs’d/bunch 6.0 MeV Ionization per bunch 230 fC Averge photon energy: 13keV Radiation damage post-study: 700GRad over 4 days, diode current dropped x2. (Comment: electronic noise was not optimized!) Prototype study, in CHESS (Slide 2) vertical position, (  m) Signal Intensity (ADC Counts) Single bunch, single pass snapshots electronic noise  photon statistics  = 142  9  m

March 5, 2008TILC08 - Sendai, JapanJim Alexander27 Beam size (  y ) measurement. Finite optical resolution: Fixed offset in  y measurement  fixed correction. 59  m here. Finite photon statistics: Stochastic error from one measurement to the next. 6.5% here* (m)(m) Prototype study, in CHESS (Slide 3) *includes electronic noise 6.5% stochastic band 59  m resolution 142  9  m observed 129  10  m actual True Beam Size Measured Beam Size (  m)

28March 5, 2008 TILC08 - Sendai, Japan xBSM Positron Optics Line Q5E HB4E Upstream Optics Box for xBSM

29March 5, 2008 TILC08 - Sendai, Japan Slit Mounting Structure Slit mount for early studies Want to explore suitable assembly for coded aperture mount ASAP Also working on mounts for other optics

30March 5, 2008 TILC08 - Sendai, Japan Collaborator Issues As stated previously, a key part of the CesrTA proposal was collaborator involvement The following slide is taken verbatim from the Joint NSF/DOE Review of the CesrTA proposal last July…

31July 16-17, 2007 Joint NSF/DOE Review of CesrTA Proposal Dealing with Challenges and Risks Experimental program is designed to deal with discoveries and changes in direction through the course of the R&D –Schedule allows for re-evaluation of key physics issues and technologies as the program proceeds Course corrections are expected along the way This makes the program robust against short term technical and/or physics surprises –Technology down-selects can be employed as data is obtained to optimize the program along the way –Program relies heavily on support from collaborators Key technical drivers for the program are: –Electron Cloud Growth Studies Chamber construction Implementation of diagnostics –Beam Dynamics Studies Issues affecting our ability to achieve ultra low emittance (see later talks) Issues affecting our implementation of high resolution emittance diagnostics (see later talks) Key assets –A well-understood machine –An experienced accelerator staff –A highly expert group of collaborators Taken from Joint NSF/DOE Review of the CesrTA Proposal July, 2007

32March 5, 2008 TILC08 - Sendai, Japan Collaboration Issues Present funding situation has several major impacts –Plans for providing experimental hardware must be revamped Wiggler chamber design and fabrication Support for coating tests –Loss of experimentalists to participate in CesrTA running Revamping run plan to accommodate a smaller number of experimenters Preserving ~240 running days during program –Loss of simulation and analysis support In US, base program support may cover portions of this Exploring Project X collaboration Hope to work closely with colleagues from KEK, CERN and elsewhere Presently working to fill remaining gaps

33March 5, 2008 TILC08 - Sendai, Japan Conclusion CESR offers –Damping wigglers meeting the ILC specification –Flexible energy and emittance range for experimental studies –Experimental studies with electrons and positrons in the identical environment –Experienced staff and well-developed tools The CesrTA program will provide –Detailed studies of electron cloud growth and validation of mitigation techniques in time for the ILC TDP-I –Beam dynamics results on electron cloud in time for the ILC TDP-I –Assurance that the ILC DR design is feasible by benchmarking our simulations with data in the relevant parameter regime