NSLS I : Challenges and upgrades on 30 year old high power RF systems Aditya Goel Brookhaven National Laboratory 08 May 2012.

Slides:



Advertisements
Similar presentations
ESLS 04 Daresbury Laboratory
Advertisements

Collaboration meeting, RAL, 4 th – 7th November 2009 Andrew Moss ASTeC Collaboration meeting, RAL, 10 th – 13 th november 2009 MICE RF Amplifier Status.
RF systems for MICE Andrew Moss The MICE RF Group and the TIARA WP7 Team Contributions include Daresbury, RAL, CERN, LBNL, LANL, FNAL, Strathclyde & Sheffield.
Linac Status Eric Prebys DOE Review, Proton Source Breakout Session July 21,2003.
KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008.
THE MICE RF SYSTEM J.F.Orrett* A.J.Moss, ASTeC, Daresbury Laboratory, WA4 4AD, UK Accelerator Science and Technology Centre
Safety Review: RF Issues Derun Li Absorber Safety Review December 9-10, 2003 Lawrence Berkeley National Laboratory Berkeley, CA
Paul Drumm 30 March 2004 MICE at RF Power System: power source, distribution Paul Drumm RAL Ambitious title!
Proton Source Workshop December 7 & 8, 2010 John Reid December 8, 2010.
DESIGN OF A HIGH POWER TEST STAND FOR ESS SPOKE CAVITIES
Beam loading compensation 300Hz positron generation (Hardware Upgrade ??? Due to present Budget problem) LCWS2013 at Tokyo Uni., Nov KEK, Junji.
NOvA meeting PIP Update W. Pellico. PIP Goals and Scope (Provided in 2011 – Directorate S. H. / DOE Talk ) Goals: Specific to the issues surrounding the.
Plan For Tests of PA/tube at 2 nd Harmonic Frequencies Robyn Madrak C. Y. Tan.
Status of 325MHz coupler S. Kazakov 11/29/ MHz coupler structure.
Andrew Moss ASTeC 7 th December 2011 MICE RF System.
Front End Test Stand Klystron Commissioning Alan Letchford UKNF Plenary Meeting 22 nd April 2009.
WAO, Trieste, 24th - 28th September 2007 An Overview of the Reliability and the Fault Trends of the SRS Cheryl Hodgkinson Daresbury Laboratory Synchrotron.
1 MICE RF Daresbury Laboratory Support Joe Orrett - ASTeC.
RF power & FPC status Eric Montesinos, CERN BE-RF on behalf of all people involved, great thanks to all of them !
R&D proposals for EuCard 2 EuCard2, April 21Steffen Döbert, BE-RF  SRF basic research (W. Weingarten)  CTF3 and CTF3+, possible infra - structure for.
 Installation: equipment, waveguides, water cooling, local cabling  Upgrade of LEP equipment  Contract follow up: new klystrons, spare circulators.
A U.S. Department of Energy Office of Science Laboratory Operated by The University of Chicago Argonne National Laboratory Office of Science U.S. Department.
1 Kenneth Osborne, 9/14/07 Inter Group communications at the Advanced Light Source. Overview of the different methods of communication between different.
F Project X Overview Dave McGinnis October 12, 2007.
February 17-18, 2010 R&D ERL Alex Zaltsman R&D ERL High Power RF Systems Alex Zaltsman February 17-18, 2010 High Power RF Systems.
Neutrino Factory Workshop, IOP, 28th October 2003 RF Systems David M Wilcox.
Andrew Moss ASTeC CM32 9t h February 2012 RAL MICE RF System.
Anders Sunesson RF Group ESS Accelerator Division
Development of the Room Temperature CH-DTL in the frame of the HIPPI-CARE Project Gianluigi Clemente,
Ding Sun and David Wildman Fermilab Accelerator Advisory Committee
Solid State RF High Power Amplifier Developments at SOLEIL Ti RUAN, on behalf of SOLEIL RF Group CWRF10 CELLS-ALBA Barcelona Spain May
Peter Hülsmann, GSI RF-Group, Tel: Task SIS18-1: h=2 Cavity P. Hülsmann GSI, Gesellschaft für Schwerionenforschung.
14th ESLS RF Workshop ELETTRA / Trieste, Italy / 2010 September The Elettra Storage Ring and Top-Up Operation Emanuel Karantzoulis.
Eric Montesinos - CERN - First SPL collaboration meeting - CERN December 11th 2008 First SPL collaboration meeting Experience with the LHC Main power Coupler.
1 BROOKHAVEN SCIENCE ASSOCIATES 2009 DOE Accelerator Safety Workshop BNL S-band LINAC Fire Safety Concerns August 19, 2009 A. Ackerman.
2010 Accelerator Safety Workshop August 18, 2010 Lessons Learned Breakout A. Ackerman.
704 MHz warm cavity November 4, 2015 A.Zaltsman: SRF & warm RF components for LEReC1  A single cell 704 MHz warm cavity is used to correct the beam energy.
ALBA RF Amplifiers based on IOTs CWRF08 - CERN, March 2008 Michel Langlois & Paco Sanchez 1 Michel Langlois & Paco Sanchez.
Comparison of Fermilab Proton Driver to Suggested Energy Amplifier Linac Bob Webber April 13, 2007.
June 3, 2004G.W.Foster - Proton Driver Proton Driver Project Development, Tactics & Strategy G. W. Foster Fermilab User’s Meeting June 3, 2004.
CWRF 2008, Geneva, March Alessandro Fabris on behalf of the Elettra RF Group Sincrotrone Trieste, Trieste, Italy. Elettra RF System Upgrade:
Operational experience of high-power RF at Diamond Light Source
Ingot Niobium Workshop RF Sources Andrew Kimber 4 th December 2015 Thomas Jefferson National Accelerator Facility is managed by Jefferson Science Associates,
The LHC RF Power Systems Skip the intro… CWRF08 workshop - March'08 1 Presented by : Luca Arnaudon Slides by : Olivier Brunner & Luca Arnaudon Important.
ATC / ABOC 23 January 2008SESSION 6 / MTTR and Spare Parts AB / RF GROUP MTTR, SPARE PARTS AND STAND-BY POLICY FOR RF EQUIPMENTS C. Rossi on behalf of.
CW and High Average Power Workshop BNL The Diamond Storage Ring IOT based High Power Amplifier Morten Jensen on behalf of the SR RF Group.
ESLS-RF Trieste, September 29-30, Åke Andersson RF systems for the MAX IV rings Åke Andersson On behalf of the MAX-lab RF team.
650 MHz Solid State RF Power development at RRCAT
Power couplers Timergali Khabiboulline (FNAL) FNAL-LBNL meeting on NGLS April 13, 2012.
New MI Cavity Progress and Plans 2010 Joseph E. Dey Project X Collaboration Meeting September 8, 2010.
ALBA RF Systems Francis Perez.
Booster High Power RF at PIP-II Era John Reid February 18, 2014.
High-efficiency L-band klystron development for the CLIC Drive Beam High-efficiency L-band klystron development for the CLIC Drive Beam CLIC workshop,
DESIGN OF A 9MHZ 15KW CW AMPLIFIER FOR RHIC Shane Dillon CTO.
High Power RF Systems for 2-8 GeV Fast Cycling Synchrotron PROJECT X (ICD-2) John Reid September 11, 2009.
A CW Linac scheme for CLIC drive beam acceleration. Hao Zha, Alexej Grudiev 07/06/2016.
Operation Status of the RF Systems and Taiwan Photon Source
Status of the ALS and APEX RF Systems at LBNL RF Group: K. Baptiste, S. Kwiatkowski (retired), Q. Du, M. Vinco, J. Julian (retired) ME Group: P. McKean.
Status and New Developments of RF Systems of ALBA
6th CWRF 2010 Workshop - ALBA, May 4, 2010
Status of the ALS and APEX RF Systems at LBNL
Developments of High CW RF Power Solid State Amplifiers at SOLEIL
SPS TWC 200 MHz Super Proton Synchrotron Travelling Wave Cavities 200 MHz 4 x 1.0 MW cw 25 years of experience.
SNS Fundamental Power Coupler History
CEPC RF Power Sources System
RF systems introduction
Status and New Developments of ALBA RF Systems
RF introduction Anders Sunesson RF group leader
Status and New Developments of ALBA RF Systems
IOT operation in the SPS Long term experience TWC 800 MHz
Presentation transcript:

NSLS I : Challenges and upgrades on 30 year old high power RF systems Aditya Goel Brookhaven National Laboratory 08 May 2012

Summary  Current description of the system.  Upgrades  Challenges  Questions

System Overview  Four electron beam accelerators Injector Systems – Linac and Booster Ring Systems – VUV and X-Ray Typical uptime of 97%

System Overview: LINAC  3 Accelerating structures  3x20 MW Pulsed Klystrons GHz LINAC Tank1 Klystron 20MW Kly1 1kW 1W RF Source Klystron 20MW Kly2 Klystron 20MW Kly3 Buncher LINAC Tank2 LINAC Tank3 90 Hybrid Magic Tee Phase Shifter Coupler

System Overview: Booster  1 Accelerating Cavity  3 kW CW Tetrode MHz RF Processor 100W 3kW RF Cavity

X-Ray Ring: System Overview  4 Accelerating Cavities  5x125kW CW Tetrode MHz  XRF2 System combines 2x125kW systems using a hybrid  Beam Current and Energy – 2800 MeV

System Overview: VUV Ring  2 Cavities – Fundamental and Harmonic  50kW Tetrode Based MHz  5kW Solid state based MHz (4 th Harmonic)  Beam Current and Energy – MeV RF Processor 100W 3kW 50kW RF Cavity Harmonic Cavity Circulator

Challenges and Upgrades  Driving Factors Reliability Obsolescence Fatigue and aging Soft challenges

Reliability  Major driver for upgrades  24x7 facility with strong emphasis on uptime  DOE mandates 90% uptime BNL aims for 95%  Regular maintenance and upgrades needed to maintain high reliability.  Several upgrades over last 30 years.  Major upgrades affecting RF systems covered here

Reliability: Booster  Booster Cavity Upgrade Original cavity was a coaxial T cavity design The cavity was prone to arcing & vacuum leaks New cavity installed in 1989

Reliability: X-Ray  Highest power CWRF systems at facility  Several upgrades to improve reliability of systems  Original amplifier design by RCA  Unsatisfactory performance and evaluation of alternative vendors yielded Eimac as the second provider of amplifiers.  Significantly improved stability, power output and tube lifetime prompted decision to change all amplifiers to Eimac

Reliability: X-Ray  Eimac improvements Gradual improvements over last 25 years Better high power contact area Better Thermal Management Ferrite tiles to get rid of 1GHz mode All these improvements have greatly increased system stability

Reliability: X-Ray Stiffen sides to prevent bowing Heat-sinks to better combat temp rise Plate line chimney water cooling Boron-nitride window to cool coax inner conductor at amplifier output Knife edge on the certain high current contacts spring fingers on amplifier front door Thicker silver plated contact area Ferrite Tiles to get rid of 1GHz mode

Reliability: X-Ray  Addition of hybrid system on XRF2 amplifier Original intention was to reduce loading on other amplifiers Better isolation between cavity and amplifier Better cavity input coupler re-designed for higher power acceptance Beryllium Oxide window on cavity input However decision was made to go to 2.8GeV Despite complicated controls and near double the amount of equipment, XRF2 system reliability has been comparable to a single amplifier system.  Modular Solid State driver amps and circulators on 3 systems Reduced amount of equipment and spares Reduced maintenance and troubleshooting time.

Reliability: X-Ray  Upgrade to full Copper cavities Original cavity copper clad steel Original cavity had problems with multi-pactoring and vacuum leaks No welding joint on critical pieces No vacuum to water interface

Reliability: VUV  VUV 50kW amplifier Original design installed in xray ring amplifier Tube lifetime was short Severe problems with drift, oscillations and sparking inside the tube. Cooling design was not adequate No other viable alternative – at that time Decision was made to redesign tube since it was being used on X-Ray and UV ring systems

Reliability: VUV  VUV 50kW tube redesign Joint effort between BNL and vendor (RCA) Redesign of grid structure for better mechanical and thermal stability Blackening of anode for better thermal conductivity

Reliability: VUV  Upgrade of 211 MHz VUV harmonic cavity amplifier Original Townsend amplifier prone to drifts, overheating and controls problems Replaced by a multi module Solid State amplifier in 1996 Only SS amplifier powering a cavity directly (through circulator) Performance has been satisfactory compared to previous amplifier

Obsolescence  Second major reason for upgrades  Usually forced upgrade to ensure future maintainability.  Currently we see more problems with low level controls and diagnostics  For vacuum tubes it is difficult to find vendors that provide good tube rebuild services.  Rebuilders committing to “best effort” services only. Does not instill confidence in future availability of services.

Obsolescence  Quality of rebuilds is a major issue – recent rebuilds on our X-Ray tubes have required very drastic changes to operating parameters to extract satisfactory performance  Our recent klystron rebuild failed twice before we received a working spare.  Manufacturers phasing out entire product lines makes spares availability very difficult. Requires us to stock a large inventory of spares.  Due to industry evolution and acquisitions locating documentation and technical support has become a major challenge.  Frequently vendors will end support or refuse to support product lines of acquired companies.

Fatigue and Aging  Usually results in catastrophic failure  Even with proper PM’s and replacements some equipment will fail prematurely.  Thermal and mechanical fatigue of High power components is a major failure mode Recently we had to “patch” a vacuum leak in our high power RF window on XRF System We found loose coaxial bullets with arc marks in high power feed-lines.

Fatigue and Aging  Age related HV insulation failure Not very easy to spot and troubleshoot We notice more failures on pulsed systems compared to our CWRF systems  In general we have had to increase our inspection and scrutiny as the systems have aged Tube sockets are a prime candidate

Soft Challenges  Usually driven by changes in policy or management  Safety and Regulatory changes Equipment and devices acceptable 30 years ago are no longer viable Ban of PCB’s required us to redesign our modulators and filtering capacitors Ignitron devices using mercury had to be addressed Safety and LOTO procedures had to be reviewed and re- written. Adoption of new fire safety rules also required us to implement fixes

Soft Challenges  Budget constraints Cuts in operational time and maintenance activities Funds availability scarce for upgrades  Loss of expertise Personnel Changes Retirements Retraining

Acknowledgements  Roy D’ Alsace  Gloria Ramirez  Joseph Papu  Peter Davila  James Rose  Douglas Durfee  Christopher Sorrentino  Kenneth Pedersen  Michael Fulkerson

Questions?