1 Slow Global Orbit Feedback at Pohang Light Source (PLS) Heung-Sik Kang Pohang Accelerator Laboratory Pohang, Korea.

Slides:



Advertisements
Similar presentations
Slide: 1 Welcome to the Non Linear Beam Dynamics Workshop P. Elleaume Non Linear Beam Dynamics Workshop, ESRF May 2008.
Advertisements

SPEAR3 short pulse development J. Safranek for the SSRL accelerator physics group* Outline: Timing mode fill patterns Short bunches –Low alpha Bunch length.
FAST ORBIT CORRECTION AT THE ESRF Eric Plouviez on behalf of: J. Chavanne, J.M. Koch, J.L. Pons, F. Uberto, L. Zhang.
K. Balewski (DESY)IWBS Conceptual Design of the PETRA III Orbit Feedback K. Balewski, H.T Duhme, J. Klute, I. Krouptchenkov, R. Neumann, G. K. Sahoo,
1 BROOKHAVEN SCIENCE ASSOCIATES NSLS-II Stability Workshop April , 2007 NSLS-II Electrical Systems G. Ganetis NSLS-II Electrical Systems NSLS-II.
Searching for Quantum LOVE at the Australian Synchrotron Light Source Eugene Tan On behalf of Rohan Dowd 120/10/2010Eugene Tan – IWLC 2010, Genega ASLS.
Alignment and Beam Stability
SESAME Synchrotron Light for Experimental Science and Applications in the Middle East JSPS Asien Science Seminar Synchrotron Radiation Science Dieter Einfeld.
Pohang Accelerator Laboratory POSTECH EPICS Collaboration Meeting RICOTTI, Tokai, JAPAN The status of PLS EPICS application EPICS collaboration.
Beam Instrumentation for Orbit Stability I. Pinayev.
Characterization of Fast Orbit Feedback System Om Singh, APS, ANL NSLS-2 Beam Stability Workshop BNL, April 18-20, 2007.
IWBS 2004 PSI, Grinderwald, Switzerland 6-10 December Orbit Stability: Recent Activities at ELETTRA, D. Bulfone Orbit Stability: Recent Activities.
NSRRC XBPM and Beam Stability Mini Workshop 2008/09/11~12 cckuo-1 TLS and TPS Vertical Beam Size Control and Beam Stability Issues C.C. Kuo NSRRC XBPM.
June 14th 2005 Accelerator Division Overview of ALBA D. Einfeld Vacuum Workshop Barcelona, 12 th -13 th September 2005 General 10 th September 2005.
12/6/2004ALS, C. Steier, IWBS IWBS 2004: ALS Facility Report Christoph Steier, A. Biocca, M. Chin, E. Domning, G. Portmann, D. Robin, T. Scarvie,
June 14th 2005 Accelerator Division Overview of ALBA D. Einfeld Vacuum Workshop Barcelona, 12 th -13 th September 2005 General 10 th September 2005.
1 BROOKHAVEN SCIENCE ASSOCIATES NSLS II: the Accelerator System Briefing Conventional Facilities Advisory Committee May 8 - 9, 2007 Satoshi Ozaki Director,
Photon Beam Position Monitors and Beam Stability at the Swiss Light Source E. van Garderen, J. Krempaský, M. Böge, J. Chrin, T. Schmidt Paul Scherrer Institute,
Technical Challenges and Concerns S. Sharma and R. Alforque, R. Beuman, C. Foerster, E. Haas, E. Hu, P. Montanez, P. Mortazavi, S. Pjerov, J. Skaritka,
Status of the Diamond Light Source R. Bartolini Diamond Light Source Ltd and John Adams Institute, University of Oxford ILCW CERN, Geneva, 20 th October.
Orbit Control For Diamond Light Source Ian Martin Joint Accelerator Workshop Rutherford Appleton Laboratory28 th -29 th April 2004.
Activities on the Orbit Feedback System for the Super-SOR Light Source SRL-ISSP, University of Tokyo Norio Nakamura 3rd International Workshop on Beam.
E. Karantzoulis - BESSY, June Elettra2.0-The next generation Emanuel Karantzoulis Circumference m 12 fold symmetry Energy 2 (& 2.4 GeV.
Simulation and Experimental Results of SSRF Top-up Operation Haohu Li, Manzhou Zhang SSRF Top-up Workshop, Melbourne
1 BROOKHAVEN SCIENCE ASSOCIATES NSLS II: Accelerator System Overview NSLS II Advisory Committees October 18/19, 2006 Satoshi Ozaki.
3rd International Workshop on Beam Orbit Stabilization - IWBS2004 December 6-10, 2004 Hotel Kirchbühl, Grindelwald, SWITZERLAND Orbit Stabilization at.
1 BROOKHAVEN SCIENCE ASSOCIATES Issues on Closed Orbit Feedback for NSLSII NSLS-II Stability Workshop April 18-20, 2007 Li-Hua Yu.
1 BROOKHAVEN SCIENCE ASSOCIATES Storage Ring Commissioning Samuel Krinsky-Accelerator Physics Group Leader NSLS-II ASAC Meeting October 14-15, 2010.
1 Proposal for a CESR Damping Ring Test Facility M. Palmer & D.Rubin November 8, 2005.
February 2010 ALBA Synchrotron Light Source Francis Perez.
28-May-2008Non-linear Beam Dynamics WS1 On Injection Beam Loss at the SPring-8 Storage Ring Masaru TAKAO & J. Schimizu, K. Soutome, and H. Tanaka JASRI.
Beam stability in damping ring - for stable extracted beam for ATF K. Kubo.
14th ESLS RF Workshop ELETTRA / Trieste, Italy / 2010 September The Elettra Storage Ring and Top-Up Operation Emanuel Karantzoulis.
1 BROOKHAVEN SCIENCE ASSOCIATES NSLS II: the Accelerator System Briefing Experimental Facilities Advisory Committee May 10, 2007 Satoshi Ozaki Director,
Automatic Machine Review Dec 2015 MAX IV Storage Rings Automation Pedro F. Tavares.
Experience Laurent S. Nadolski Accelerator Physics Group On behalf of the Sources and Accelerator Division.
Canadian Light Source Commissioning Progress CLS Annual Users Meeting –
Advanced Optics Control, CERN, Masamitsu Aiba, PSI Recent optics measurements at SLS M. Aiba, M. Böge, Á. Saá Hernández, D. Mayilyan and.
Photon Beam Position Monitors and Beam Stability at the Swiss Light Source Elsa van Garderen March 12 th, 2008.
Beam Physics Issue in BEPCII Commisionning Xu Gang Accelerator physics group.
LCWS, UTA, Reaching ultra-low emittance at SLS through (systematic and) random optimization LCWS 2012 Joint CLIC/ILC Working Group – Damping.
4. Operations and Performance M. Lonza, D. Bulfone, V. Forchi’, G. Gaio, L. Pivetta, Sincrotrone Trieste, Trieste, Italy A Fast Orbit Feedback for the.
Machine Operation and Studies at SSRF Wenzhi ZHANG Dec. 16, 2013 Spain.
Workshop on Accelerator R&D for Ultimate Storage Rings – Oct Nov.1 – Huairou, Beijing, China A compact low emittance lattice with superbends for.
1 Jean-Claude DENARD Workshop on Accelerator R&D for Ultimate Storage Rings Version 2.0 ORBIT FEEDBACK SYSTEMS and XBPMs J-C. Denard, N. Hubert * and L.
C. Steier, USR 2012, Feedbacks for USR, Workshop on Accelerator R&D for Ultimate Storage Rings : Beijing / IHEP, October 2012 Feedbacks for Ultimate.
1 BROOKHAVEN SCIENCE ASSOCIATES Beam Stability Overview NSLS-II CFAC Meeting May 8, 2007 S. Krinsky.
Anticipated Limits on Machine Stability and some Consequences on Machine and Beamline Designs Jean-Claude Denard Workshop on Accelerator R&D for USRs Hairou,
Accuracy of the orbit measurement by KEKB BPM system for the study of ILC damping ring H. Fukuma (KEK) Requirement for the accuracy of BPM data.
Fast Global Orbit Feedback for the Australian Synchrotron Eugene Tan Accelerator and Operations 13/12/20101 ACAS Workshop on Accelerator Feedback Systems.
Ultra-low Emittance Coupling, method and results from the Australian Synchrotron Light Source Rohan Dowd Accelerator Physicist Australian Synchrotron.
ESLS Workshop Nov 2015 MAX IV 3 GeV Ring Commissioning Pedro F. Tavares & Åke Andersson, on behalf of the whole MAX IV team.
Operation Status of the RF Systems and Taiwan Photon Source
MACHINE OPERATION AT ALBA Montse Pont, CELLS-ALBA 16-18/12/2013.
Report Technical Director Storage-Ring-Installation Completed
Weiming Guo Accelerator Physics Group / ASD Advanced Photon Source
Experiments on Fast Ion Instability at PLS
Diamond Light Source Status and Future Challanges
STATUS OF THE ALBA SYNCHROTRON LIGHT SOURCE: FROM COMMISSIONING TO OPERATION M.Pont, CELLS-ALBA
Status of the ASTRID2 facility
Orbit Control For Diamond Light Source
Coupling Correction at the Australian Synchrotron
SOLEIL Fast Orbit Feedback System
Commissioning the Fast Orbit Feedback System at SSRF
Machine Operation and Progresses in SSRF
Operation Progress and Upgrade in SSRF
Beam-Based Alignment Results
SPEAR3 Lower Emittance & Nonlinear Dynamics
Fast Orbit Feedback at the SLS
Proposal for a CESR Damping Ring Test Facility
Presentation transcript:

1 Slow Global Orbit Feedback at Pohang Light Source (PLS) Heung-Sik Kang Pohang Accelerator Laboratory Pohang, Korea

2 Brief History of PLS Aerial View of PAL Project started Apr Ground-breaking Apr GeV Linac commissioned Jun Storage ring commissioned Dec User’s service started Sept Energy ramping to 2.5 GeV Sept GeV injection Nov

3 Pohang Light Source  Beam Energy2.5GeV  Beam Current200mA  LatticeTBA  Superperiods12  Circumference280 m  Emittance18.9 nm-rad  Tune14.28 / 8.18  RF Frequency500 MHz  Energy spread8.5 x GeV Linac / Storage Ring Beam SizeOrbit Stability HorizontalVerticalHorizontalVertical Bending Magnet 230  m24  m23  m2.4  m Insertion Devices 455  m35  m45  m3.5  m PLS Orbit Stability Requirements

4 Orbit Feedback  Slow global orbit feedback (SOFB)  Improvement of Power Supplies  V: 12 bit -> 20 bit resolution (22 ea) New power supply with the controller developed in BESSY II  H: 12 bit -> 16 bit (22 ea) modification of existing power supplies  Operational since October 2004  Feedback Speed: 4 sec  SVD algorithm, MATLAB / EPICS  Feedforward correction for ID is under test  Fast global orbit feedback (FOFB) Under consideration March 2004, w/o SOFB For 9 days 200  m Frequency Spectrum of BPM reading High frequency movement RMS-y

5 MATLAB GUI for Slow Global Orbit Feedback  The orbit feedback algorithm uses the SVD (singular value decomposition) method.  Use the Matlab Channel Access to EPICS IOC of BPMs and correctors  The GUI displays the response matrix, the spectrum of singular values, the real time orbit, and the correction kick.

6 Correctors and BPMs for SOFB 9 BPMs & 6 Correctors /sector  Totally, 108 BPMs and 70 correctors in each plane BPM electronics: Bergoz MUX BPM Insertion Devices (6) –Undulator: U7, EPU6, U10, In-Vacuum Revolver (min. gap: 5 mm) –Multipole Wiggler: HFMX, HFMS P 1 C2 C3 C4 C5 C6 C1 P 9 P 8 P 7 P 6 P 5 P 4 P 3 P 2 ID  SOFB uses - 2 correctors (C1 & C2) / sector -> 22 correctors in each plane - 6 BPMs / sector - Current dependence table for BPM electronics Horizontal plane:16 bit resolution -> 0.06  rad/ 1 bit Vertical plane:20 bit resolution ->  rad/ 1 bit One sector

7 Orbit Variations in SOFB during USER RUN (Nov. 16 – 25, 2004) Reference orbit is re-set For one day For 10 days Reference orbit is re-set at 150 mA after refill. Current dependence data of BPM electronics is referenced to the BPM reading at 150mA 1. The number of correctors is not enough for correction 2. To effectively compensate the BPM electronics’ current dependence RMS-y RMS-x RF freq

8 False BPM Reading BPM Reading 1) Real Beam Position change 2) BPM Electronics’ dependence on Ambient temperature 3) BPM Electronics’ dependence on Beam current 4) Chamber movement 2  m 120 mA 180 mA - BPM electronics problem: Gain drifts and non- linearities Beam current BPM reading  Current Dependence table is used to subtract the false value from the BPM reading for SOFB  But, chamber movement is not compensated.  Compensation of false BPM reading is absolutely necessary in order to minimize the false motion by orbit feedback.  Ambient temperature dependence can not be compensated, thus should be minimized.

9 Beam Current Dependence of BPM electronics Horizontalvertical BPM reading change between 120mA and 180mA (not include the bad BPMs) X – rms : 2.9  m Y – rms : 5.0  m Non-linearity of current dependence  Different Change rate of current dependence low current rage: 153 – 112 mA (blue line) high current range: 188 – 153 mA (green line)  Current Dependence table for SOFB : red line ( mA) Linear rate of current dependence [um/mA] 112 mA 188 mA 153 mA

10 Patterns of BPM ’ s Intensity dependence Chamber Motion + BPM electronics BPM 7-5 Y 2  m BPM 6-4Y 10  m BPM 9-2Y BPM 9-5Y 5  m 12-8Y Temperature of Vacuum Chamber in straight section ( Sep. 14 – 15, 2004, Bad Orbit condition) After the orbit correction

11 BPM Chamber Movement  vacuum chamber moves due to the change of synchrotron radiation heat load  dependent on orbit  Look-up table is not easy to implement. 2.0 GeV 400 mA 2.5 GeV 200 mA 2.5 GeV 250 mA Synchrotron radiation power 115 kW128 kW161 kW Photon power / sector 9.6 kW10.6 kW13.4 kW Photon Fan BM Photon Stop One sector

12 Change of BPM Reading in SOFB 7-6 Y 9-5 Y BPM 9-5Y 7-5 Y 9-5 Y SOFB OFF SOFB ON 5  m 1  m 5  m Beam current BPM with a large chamber movement BPM with a negligible chamber movementBPM with a small chamber movement

 m 10  m 2  m 10  m 4  m x y BPM BPM Chamber Movement Digital Position sensor (accuracy: < 100 nm) Beam 2.5 GeV sector number Measurement of BPM Chamber Movement 200mA

14 Variations of Corrector Currents in SOFB Very similar to BPM chamber movement BPM electronics' current dependence looks compensated well. 2CV1 3CV2 3CV1 4CV2 9CV2 Beam current

15 Ambient Temperature Dependence of BPM Electronics ( BPM reading oscillation) Cooling Fan OFF BPM 8-2Y 5  m 0.02 V AGC The same oscillation was observed in the ambient air temperature in the control shed where the BPM electronics is. BPM electronics Must be influenced by the ambient temperature. One BPM electronics module shows Dependence on Ambient temperature : 1.4  m /  C Ambient temperature in control shed should be well controlled. BPM 7-4Y 18:00 Dec. 6 2 hours 2  m

16 BPM’s intensity Dependence limits the SOFB performance. Solution is TOP-UP! BUT, Decided not to use it until …. Because 1. For Linac, Injection efficiency is not so good compared to Booster. Synchronization of RF between SR and Linac is required. 2. We will start SASE-FEL project in No. 1 Priority of Linac is changed…

17 PAL XFEL Project Period: Budget: 80 M$

18 How to Compensate Chamber Motion in SOFB Real-time measurement of BPM Chamber Motion for all BPMs (108 ea) by Digital position sensor or LVDT (Budget allocated in 2005) Chamber position is monitored with respect to Girder, which is equivalent to Quad because Girder is very rigid. EPICS Database Compensate the chamber motion from BPM reading in SOFB (data refresh time : 1-3 minutes)  Neglect the Girder motion with respect to ground, and the Girder to Girder differences  Quad does not move as the Beam loading changes.  Care about the orbit with respect to Quad. QM invar QM Chamber

19 SOFB for Insertion Device BPM 4-3Y 2  m FB ONFB OFF 13:41 H: 16-bit correctors V: 20-bit correctors Vertical orbit changes up to 6  m in rms when the EPU gap is moving between 20 and 25 mm. Feedforward correction is required. Due to EPU gap change Beam current

20 Feedforward for EPU6 New Correctors for Feedforward CM1CM1 PM1PM1 CM2CM2 PM2PM2 Q1Q2 CM3CM3 Q3 PM3PM3 BM1 PM4PM4 SDQ4Q5SF PM5PM5 CM4CM4 Q6BM2 PM6PM6 Q6D CM5CM5 PM7PM7 SFD Q5DQ5D Q4DQ4D SDD PM8PM8 BM3 PM9PM9 Q3DQ3D CM6CM6 Q2DQ2D Q1DQ1D ID Feed-forward correction - correctors: 1CM6 and 2CM3  just done for test New correctors for Feedforward  ready for test - speed: 10 Hz

21 EPU6 Feed-forward Correction Feedforward speed: 10 Hz Vertical correctors: 1CM6 and 2CM3 Feedforward table 5 th degree polynomial for fitting

22 Summary Achieved orbit stability by SOFB - short term (1 hour) : < 1  m - long term (12 hours) : < 3  m BPM Chamber movement due to Synchrotron Radiation heating mainly limits the SOFB performance. Real-time measurement of BPM Chamber Motion for all BPMs (108 ea) Reduction of BPM Noise –Feedback speed : 4 sec  2 sec 70 correctors in vertical plane  20-bit resolution Improvement Plan of SOFB in 2005