Renovation of the 200 MHz RF system LLRF issues. Cavities redistribution 26 October 201114th LIU-SPS Coordination Meeting 2  2011 : 4 cavities 2 x 4.

Slides:



Advertisements
Similar presentations
EMMA RF System Summary RF Requirements (S Berg): Aperture: –Aperture 34.7 mm (min) –Dispersion effects may increase by 3 – 4 mm Frequency: –Frequency range.
Advertisements

RF Specification discussion MICE RF workshop 16 th April 2012.
New 200 MHz and 800 MHz amplifiers
Op-Amp- An active circuit element designed to perform mathematical operations of addition, subtraction, multiplication, division, differentiation and.
Frequency modulation and circuits
Breakdown Rate Dependence on Gradient and Pulse Heating in Single Cell Cavities and TD18 Faya Wang, Chris Nantista and Chris Adolphsen May 1, 2010.
11/27/2007ILC Power and Cooling VM Workshop Mike Neubauer 1 RF Power and Cooling Requirements Overview from “Main Linac Power and Cooling Information”
CHAPTER 3 MICROWAVE ‘O’ TYPE TUBES
Areal RF Station A. Vardanyan RF System The AREAL RF system will consist of 3 RF stations: Each RF station has a 1 klystron, and HV modulator,
BEPCII RF POWER SYSTEM RF group, IHEP Sep ~ April 1.The 1 st transmitter had finished installing,commissioning and SAT (Site Acceptance Test).
HIGH POWER SYSTEMS FOR WIND PROFILER K. P. Ray K. P. Ray Society for Applied Microwave Electronics Engineering & Research IIT campus, Powai, Mumbai-400.
Areal RF Station A. Vardanyan RF System The AREAL RF system will consist of 3 RF stations: Each RF station has a 1 klystron, and HV modulator,
Progress of the sub-harmonic bunching system (i.e. upgrading progress of BEPCII present bunching system) Pei Shilun for the SHBS team Accelerator center,
RF Synchronisation Issues
DESIGN OF A HIGH POWER TEST STAND FOR ESS SPOKE CAVITIES
Potential improvements of the PS 10 MHz cavities driving amplifier G. Favia Acknowledgments: V. Desquiens, F. Di Lorenzo S. Energico, M. Morvillo, C.
Strategy for SPS 200 MHz LLRF upgrade (1)  Each of the four cavities (2x 5 sections, 2x 4 sections):  1-T Feedback (loop around cavity and amplifier)
Andrew Moss ASTeC 7 th December 2011 MICE RF System.
RF Distribution Alternatives R.A.Yogi & FREIA group Uppsala University.
RF power & FPC status Eric Montesinos, CERN BE-RF on behalf of all people involved, great thanks to all of them !
Announcements mid-term Thursday (Oct 27 th ) Project ideas to me by Nov 1 st latest Assignment 4 due tomorrow (or now) Assignment 5 posted, due Friday.
Amplitude Modulation 2.2 AM RECEIVERS
David Regidor, Moisés Weber (CIEMAT, Madrid, Spain) The IFMIF-EVEDA Accelerator Prototype will be a 9MeV, 125mA CW deuteron accelerator to validate the.
CommunicationElectronics Principles & Applications Third Edition Chapter 6 Radio Transmitters ©2001 Glencoe/McGraw-Hill Louis E. Frenzel.
AAC February 4-6, 2003 Protons on Target Ioanis Kourbanis MI/Beams.
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.
Travelling Wave Tube For Broadband amplifier helix TWTs (proposed by Pierce and others in 1946 ) are widely used For High average power purposes the.
Anders Sunesson RF Group ESS Accelerator Division
PSB C04 RF system Consolidation or upgrade? M. Paoluzzi – CERN BE-RF 11/23/20151.
13 th April 2007FFAG 07 Carl Beard EMMA RF System Carl Beard, Emma Wooldridge, Peter McIntosh, Peter Corlett, Andy Moss, James Rogers, Joe Orrett ASTeC,
Amplifiers Amplifier Parameters Gain = Po/Pi in dB = 10 log (Po/Pi)
Almost 40 years of operation with tetrodes in the CERN-SPS CWRF workshop 2014, Trieste Eric Montesinos, CERN-RF, on behalf of RF-SPS team CWRF workshop,
CLARA Gun Cavity Optimisation NVEC 05/06/2014 P. Goudket G. Burt, L. Cowie, J. McKenzie, B. Militsyn.
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
RF scheme of electron linear accelerator with energy MeV Levichev A.E. Budker Institute of Nuclear Physics SB RAS.
ESS RF System Design Stephen Molloy RF Group ESS Accelerator Division SLHiPP2 4-May-2012.
Commissioning of the ALBA IOT-Transmitters Paco Sanchez - 14th ESLS RF - ELETTRA, September Paco Sanchez, RF Group, CELLS (Consortium for.
ALBA RF Amplifiers based on IOTs CWRF08 - CERN, March 2008 Michel Langlois & Paco Sanchez 1 Michel Langlois & Paco Sanchez.
SPS point 3 New RF building LIU-SPS-200 MHz Power Upgrade April 19, 2011Eric Montesinos / CERN-BE-RF-SR.
SPS 200 MHz RF Upgrade Eric Montesinos LIU-SPS coordination meeting 17 th December 2013.
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.
SPS point 3 LSS3 rearrangement LIU-SPS-200 MHz Power Upgrade May 26, 2011Eric Montesinos / CERN-BE-RF-SR.
SPS 200 MHz RF Upgrade Eric Montesinos LIU-SPS coordination meeting 15 th August 2012.
FREIA: HIGH POWER TEST STAND Rutambhara Yogi & FREIA Group ESS RF Group Unit Leader for Spoke Power and RF Distribution FREIA Group Unit Leader, Uppsala.
650 MHz Solid State RF Power development at RRCAT
ALBA RF System Paco Sanchez - 13th ESLS RF - DESY, 30 September Paco Sanchez, RF Group, CELLS (Consortium for the Exploitation of the Synchrotron.
ALBA RF Systems Francis Perez.
HiLumi-LHC/LARP Crab Cavity System External Review 5-6 May 2014, BNL SPS - RF Power and Coupler status Erk Jensen, Eric Montesinos, CERN BE-RF.
RF Commissioning D. Jacquet and M. Gruwé. November 8 th 2007D. Jacquet and M. Gruwé2 RF systems in a few words (I) A transverse dampers system ACCELERATING.
The Working Theory of an RC Coupled Amplifier in Electronics.
Linac RF System Design Options Y. Kang RAD/SNS/NScD/ORNL Project – X Collaboration Meeting April , 2011.
FUNCTION GENERATOR.
DESIGN STUDY November 28 th - 30 th 2005First EURISOL Design Study TOWN MEETING High Power RF Amplifiers Development at LNL Fabio Scarpa - INFN LNL.
Areal RF Station A. Vardanyan
ILC Power and Cooling VM Workshop
Test of the dressed spoke cavity
High efficiency work and MBK development for accelerators
Developments of High CW RF Power Solid State Amplifiers at SOLEIL
Longitudinal beam parameters and stability
Wideband, solid-state driven RF systems for PSB and PS longitudinal damper.
10 MHz amplifier status G. Favia
Physics design on Injector-1 RFQ
12 GHz High Power RF components requirements for CEA activities
Notkestrasse 85, Hamburg, Germany
The SPS 800 MHz RF system E. Shaposhnikova for BE/RF
CEPC RF Power Sources System
Beam dynamics requirements after LS2
Chapter 5: Active Filters
CEPC SRF Parameters (100 km Main Ring)
Presentation transcript:

renovation of the 200 MHz RF system LLRF issues

Cavities redistribution 26 October th LIU-SPS Coordination Meeting 2  2011 : 4 cavities 2 x 4 sections 2 x 5 sections + 3 spare sections  2018 : 6 cavities 4 x 3 sections 2 x 4 sections + 1 spare section Courtesy of Elena Shaposhnikova

1.7 MW amplifier, i.e 1.4 MW cavity 26 October th LIU-SPS Coordination Meeting 3  To have 1.4 MW available at the cavity input, 1.7 MW at the Final output are needed  A major improvement to present systems would be to have individual SSA drivers per PA  Taking advantage of the long experience we have with tetrodes and combiners, the solution will be 16 x PAs combined through 3 dB combiners  Four contracts :  Drivers (SSA)  Finals (SSA or Tetrodes)  Combiners (3 dB above 100 kW)  Transmission lines (coaxial, 345 mm outer) Drivers 16 SSA Final 16 PAs 3 dB combiners and power loads 120 m and 180 m Coaxial lines To cavity input 120 m away From Beam Control 1/16 splitter 1.7 MW -0.6 dB total 1.5 MW -0.2 dB 1.4 MW

16 Tetrodes vs 2048 SSA 26 October th LIU-SPS Coordination Meeting 4  Tetrodes tube costs over 20 years will be added :  20 years * 3/4 * 335 * 24 * 16 * 2 = 3’859’200 total hours  With 20’000 hours per tube = ~ 200 tubes  SSA :  + 20% to 25% additional transistors (not module)  Individual circulators are mandatory  Wall plug efficiency will be part of the adjudication  HVPS included (Tetrodes)  Losses in all SSA combiners, circulators and loads included 1.7 MW 128 x 830 W SSA FinalTetrodes (gain = 12 dB) SSA (Gain = 20 dB) Nominal ratings 16 x 106 kW = 1700 kW2048 x 830 W = 1700 kW Maximum ratings For 1400 kW at cavity input Maximum 2 faulty tubes 14 x 138 kW = 1932 kW Maximum 48 faulty modules 2000 x 891 W = 1782 kW Maximum ratings Driver 16 x 8.7 kW16 x 1.1 kW 16 x 106 kW Tetrodes 16 x

First upgrade: Present amplifiers 26 October th LIU-SPS Coordination Meeting 5 Maximum RatingsPresentFuture CW, 5 seconds650 kW700kW Pulsed, 43 kHz900 kW1100 kW Tubes per year (547’000 CHF) (629’000 CHF) Solutions Increased Filament voltageVery expensive Siemens HVPSneed a full re-cabling and an air cooling improvement Philips amplifiersair cooling plant to be modified BW -3dB Compromise to be discussed with LLRF

More Power with Present amplifiers 26 October th LIU-SPS Coordination Meeting 6  Increase filament voltages :  Very expensive (562’000 CHF -> 1’111’000 CHF per year)  Effective efficiency not tested !  Additional down time YL1530 Ufil Max peak power LifetimeTube per year Nb of stopsYL1530 Costs Additional cost Nominal900 KW25’000 hrs17 187’ %1.0 MW- 25 % ’ ’ %1.1 MW- 44 % ’ ’000 RS2004 Ufil Max peak power LifetimeTube per year Nb of stopsRS2004 Costs Additional cost Nominal800 KW20’000 hrs ’ %900 kW- 25 % ’ ’ %1 MW- 44 % ’ ’ %1.1 MW- 58 % ’ ’000

More Power with Present amplifiers 26 October th LIU-SPS Coordination Meeting 7  HVPS Siemens improvements :  Full re-cabling  Air cooling modification  Philips amplifiers improvement :  Air cooling modification  ‘pre-modifications’ during next Xmas stop to test new configuration during a MD in 2012 :  TX3 Siemens HVPS  TX5 Air cooling Siemens HVPS need an air cooling improvement Siemens HVPS need a full re- cabling with new cable spacers

More Power with Present amplifiers 26 October th LIU-SPS Coordination Meeting 8  Driver over coupled trick already used nowadays on all TXs  Maximum Power strongly proportional to BW  Driver over coupled trick already used nowadays on all TXs BW -3dB [MHz] Pout [kW]

Present amplifiers BW 26 October th LIU-SPS Coordination Meeting 9  The effective BW of the 1-Turn feedback is limited by  The TX gain BW: When the TX gain drops by ~ 20 dB, the overall loop has no more gain  The TX phase non-linearity: When the phase shift exceeds +-50 degree the overall loop gain must have dropped by more than 20 dB to keep the system stable  Conclusion: Good correction only in the band limited by +-30 deg phase non-linearity, and with an effectiveness that drops as the TX gain BW BW -3dB BW -15dB Phase distortion Siemens Line 1TX1 + TX24 sections ≥ 2.5 MHz ≥ 5 MHz+/- 3.0 MHz+/- 30 ° Line 2TX3 + TX44 sections Philips Line 3TX5 + TX65 sections ≥ 8 MHz+/- 5.0 MHz+/- 30 ° Line 4TX7 + TX85 sections

BW specifications ? 26 October th LIU-SPS Coordination Meeting 10  New plan :  Present amplifiers connected to 3 sections cavities with higher bandwidth than 4 and 5 sections as per nowadays  New amplifiers connected to 5 sections cavities  What is the acceptable BW limit ? :  For ‘Siemens’ and ‘Philips’  For new amplifiers  2018 : 6 cavities 4 x 3 sections 2 x 4 sections + 1 spare section

Operation modes (on a match power load) 26 October th LIU-SPS Coordination Meeting 11 Measurements to be made on a power load Measurements with a MHz carrier at 400 kW and a frequency sweep 20dB below carrier : Non linear phase distortion at +/- a MHz: max. +/- b° Passband at -1 dB: x.0 MHz Passband at -3 dB: y.0 MHz Passband at -15 dB: z.0 MHz Measurements to be made in CW and 10 us/43 kHz on a power load With Po = 850 kW cw With Po = 1700 kW 10 us / 43 kHz Pout vs Pin must be monotonic from zero to Po Small signal differential gain g = dPout/dPin, in the range 0.1 Po to 0.9 Po : Local slope variation max +/-15% Can vary by 3 dB maximum. Gain saturation curve Non linear phase distortion (CW): Δ φ max < 10º Non linear phase distortion curve

Operation modes (on a match power load) 26 October th LIU-SPS Coordination Meeting 12 Continuous operation 24/24 hours CW for 10 months continuously Very Long Pulses operation Fc = MHz +/- 0.5 MHz : 100% from 0 to 900 kW with rise and fall time < 0.5 µs 5 seconds ON / 5 seconds OFF AM modulation #1 Fc = MHz +/- 0.5 MHz : 100% from 0 to 900 kW with rise and fall time < 0.5 µs Repetition time 10 µs (100kHz) AM modulation #2 Fc = MHz +/- 0.5 MHz : 0 to 1700 kW with 4 MHz triangle AM 25 % in power Rise and fall time < 0.5 µs Flat top pulse and off pulse length of 11 us Repetition time 23 µs (43kHz) (and 172 kHz) This cycle for 20 second then 1 second OFF.

New RF building 26 October th LIU-SPS Coordination Meeting 13  No more ‘Power’ in BB3 Faraday Cage  Specific ‘Power’ control room in new RF building, Cavity controllers, Conditioning systems, amplifiers monitoring  BB3-FC large enough for 6 systems ?

Beam Control resources Beam Control 1’ Draft schedule 26 October th LIU-SPS Coordination Meeting 14 Authorizations Install Build new hardware Year 4Year 3Year 2Year 1Year 5 Building Services RF : Building: Year 6Year 7 Commissioning Tunnel : Build New hardware Installation phase 1 (pickups + dampers + EL + coax lines …) Installation phase 2 (cavities + pickups + CV + EL + vacuum) Cavities re-arrangement within a LS ( > 6 months) Studies (amplifiers, couplers, cavities, LLRF) Tendering (s) Studies Services

LLRF/Beam Control open issues ? 26 October th LIU-SPS Coordination Meeting 15  What is the acceptable lower BW limit ? :  For ‘Siemens’ and ‘Philips’  For new amplifiers  Technical Specifications ?  BB3-FC large enough for 6 systems ?  Is a 3 sections cavity available in new RF building earlier useful ?  Is the draft schedule still correct ?  Time table  Resources  Money  How many time for commissioning without/with beam ?  What if LS2 earlier ? (later ?)  What else ?