CRISP WP 7 SSA using a cavity combiner Michel Langlois, Pierre Barbier, Jörn Jacob Page 2 CWRF 2014 Trieste May 13-16 Michel Langlois, Pierre Barbier,

Slides:



Advertisements
Similar presentations
RFQ Tuning and RFQ Control Status
Advertisements

CHAPTER 3: SPECIAL PURPOSE OP-AMP CIRCUITS
11/27/2007ILC Power and Cooling VM Workshop Mike Neubauer 1 RF Power and Cooling Requirements Overview from “Main Linac Power and Cooling Information”
We have so far seen the structure of a differential amplifier, the input stage of an operational amplifier. The second stage of the simplest possible operational.
HIGH POWER SYSTEMS FOR WIND PROFILER K. P. Ray K. P. Ray Society for Applied Microwave Electronics Engineering & Research IIT campus, Powai, Mumbai-400.
MICE Refurbishment of CERN RF equipment for MICE M. Vretenar, CERN AB/RF.
KAGEYAMA, T. Open Meeting for Proto-Collaboration March 19, 2008.
SESAME Storage Ring RF-System
Introduction The input network of the power amplifier will be designed in the example. The network synthesized will be expanded to allow for biasing of.
Aperture-coupled Stacked Coplanar Patch Antenna Presented by: Mohamed Morsy Date: October 19,2006.
Tom Kubicki.  Booster HLRF System to be upgraded using 1kW Solid State Driver (SSD) Amplifiers.  Used to drive the 200kW Power Amplifier  Eliminates.
DESIGN OF A HIGH POWER TEST STAND FOR ESS SPOKE CAVITIES
An amplifier with a transistor that conducts during the entire 360º of the input signal cycle. Optimum class A operation is obtained by designing an amplifier.
Chapter Two: Radio-Frequency Circuits. Introduction There is a need to modulate a signal using an information signal This signal is referred to as a baseband.
Plan For Tests of PA/tube at 2 nd Harmonic Frequencies Robyn Madrak C. Y. Tan.
IC Voltage Regulator.
Electrical, Electronic and Digital Principles (EEDP)
Jörn Jacob: RF solid state amplifiers
Andrew Moss ASTeC 7 th December 2011 MICE RF System.
Collaboration meeting, DL, 19 h – 23 h October 2008 Andrew Moss ASTeC Collaboration meeting, DL, 19 th – 23 th October 2008 MICE RF distribution system.
RF Distribution Alternatives R.A.Yogi & FREIA group Uppsala University.
Modelling of TPM noise problems Greg, following discussions and measurements with David and Senerath.
Introduction to Controlling the Output Power of a Transistor Stage A load network will be designed to maximize the output power obtainable from the Mitsubishi.
RF power & FPC status Eric Montesinos, CERN BE-RF on behalf of all people involved, great thanks to all of them !
SESAME STORAGE RING RF-SYSTEM SESAME-TAC meeting Nov.2012 SESAME SR RF System – Darweesh FOUDEH.
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.
Equalisation.
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
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.
Cold Tuner test overview S1-Global at KEK 5-9 July 2010.
© 2013 The McGraw-Hill Companies, Inc. All rights reserved. McGraw-Hill 8-1 Electronics Principles & Applications Eighth Edition Chapter 8 Large-Signal.
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.
CWRF 2008, Geneva, March Alessandro Fabris on behalf of the Elettra RF Group Sincrotrone Trieste, Trieste, Italy. Elettra RF System Upgrade:
J. Jacob: RF Operation, Cav's and SSA's at ESRF
SPL waveguide distribution system Components, configurations, potential problems D. Valuch, E. Ciapala, O. Brunner CERN AB/RF SPL collaboration meeting.
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.
Slide: Sixth CW and High Average Power RF Workshop Cavity combiners for transistor amplifiers M.Langlois, J.Jacob, J.M. Mercier.
Solid State Amplifier Circuit Design Student: Branko Popovic Advisor: Geoff Waldschmidt.
BARC-IIFC collaboration meet RF Solid-state Power Amplifiers at 325 MHz RFSS, TPD, BARC.
650 MHz Solid State RF Power development at RRCAT
TIARA Workshop on RF Power Generation Uppsala, June 2013
SLAC Project-X RF Development FY12 SOW March
IIFC Meeting February 24-25, 2015, RRCAT P. R. Hannurkar, Akhilesh Jain, M. R. Lad RF Systems Division 650 MHz RF Power 1.
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.
DESIGN OF A 9MHZ 15KW CW AMPLIFIER FOR RHIC Shane Dillon CTO.
Linac RF System Design Options Y. Kang RAD/SNS/NScD/ORNL Project – X Collaboration Meeting April , 2011.
A CW Linac scheme for CLIC drive beam acceleration. Hao Zha, Alexej Grudiev 07/06/2016.
Report on Sigmaphi 75 kW RFQ Amplifier and Ferrite 75 kW Circulator Ralph Pasquinelli November 18, 2014.
Solid state RF amplifier development at ESRF 9th CWRF workshop June 2016 Michel Langlois & al. Participants:  The RF group with special thanks.
DESIGN STUDY November 28 th - 30 th 2005First EURISOL Design Study TOWN MEETING High Power RF Amplifiers Development at LNL Fabio Scarpa - INFN LNL.
High Power RF Solid State Amplifiers at FREIA
J. Jacob: RF developments at ESRF: HOM free Cu Cav. & SSA
Solid State Amplifier Development at PSI
Coaxial tunnel roof feed-through and its cooling
RF Layout 3pi/2 for Discussion
Developments of High CW RF Power Solid State Amplifiers at SOLEIL
Wideband, solid-state driven RF systems for PSB and PS longitudinal damper.
Physics design on Injector-1 RFQ
Michel Langlois & Jörn Jacob ESRF
Analog Electronic Circuits 1
Vita 83 Working Group proposal for Rugged packaging,
POWER AMPLIFIERS.
CEPC RF Power Sources System
Amplifiers Classes Electronics-II
Amplifiers Classes Electronics-II
Status and New Developments of ALBA RF Systems
Status and New Developments of ALBA RF Systems
ESRF Experience with Solid State Amplifiers and Combiners
Presentation transcript:

CRISP WP 7 SSA using a cavity combiner Michel Langlois, Pierre Barbier, Jörn Jacob Page 2 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob

CRISP WP 7 Page 3 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob THE MAIN DRAWBACK OF SSA FOR SCIENCE IS THE LARGE RATIO BETWEEN SPECIFIED RF POWER AND MODEST SINGLE MODULE POWER HENCE 2 MAIN TARGETS FOR THIS DEVELOPMENT: Decrease the footprint and volume of solid state amplifiers. Make them cheaper, i.e. decrease the €/W rating.

CRISP WP 7 Page 4 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob 5 IDEAS COULD MAKE IT HAPPEN! 1/ Make use of a cavity combiner to provide compactedness! The resonator operates in E010 mode. All modules are coupled to the resonator with fixed loops. The resonator is capacitively coupled to the waveguide. This coupling can be varied.

CRISP WP 7 Page 5 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob HOW SUCCESSFUL? diameter 2.1m height 1.37m Footprint efficiency=54.8 kW/m2 Volume efficiency =40 kW/m3 height 2.7m diameter 1.32 m Footprint efficiency=21.6 kW/m2 Volume efficiency =8.02 kW/m3 75 kW C.W.

CRISP WP 7 Page 6 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob 2/ USE OFF-THE-SHELF POWER SUPPLIES. CRISP project WP7 A 50V/10kW supply is chosen. It is available from a European manufacturer. It feeds a wing containing 6 modules. They use the 400V/ 3 phases mains. The amplifier is still in operation if one supply dies. The power derating, if any, is not known yet. Configuration for 3 wings=18 modules of 700W each

CRISP WP 7 Page 7 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob 3/ RF MODULES FEATURE PLANAR BALUNS, NO CHOKES AND NO TRIMMING PCB implementation Balun coaxial implementation Involving manpower Printed baluns, accurate capacitor values and positions make it possible to do away with trimming

CRISP WP 7 Page 8 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob 4/ RF AND D.C. DISTRIBUTION USE THE SAME SUPPORT AS THE RF MODULES. front side of a wing Including 6 RF modules + circulators + loads back side of a wing Including RF drive splitting and DC distribution

CRISP WP 7 Page 9 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob 5/ THE MODULES ARE NOT INDIVIDUALLY SHIELDED + the sole of the transistor is very close to the cooling channel. + much cheaper than individual shielding. - RF radiation originating from the circulator tabs.

CRISP WP 7 Page 10 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob ACHIEVEMENTS SO FAR A cavity combiner equipped with 3 wings of 6 modules has been built and tested on a 50 Ω dummy load.

CRISP WP 7 Page 11 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob GAIN AND PHASE DISTRIBUTIONS CRISP project WP7 The modules were hand made. It caused a poor reproducibility of the matching capacitors positions. The transistors (NXP BLF578) came from different batches ordered at different times. Will these modules still combine harmoniously?

CRISP WP 7 Page 12 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob AMPLIFIER PERFORMANCES Test conditions: Idq=2*100mA per module (nearly class B) Vds=50V 15l/min per wing 63%=Prf/(Vds*ΣId)=drain efficiency The efficiency of a class B amplifier is bad at low output level. If the RF power has been overestimated, the number of wings plugged on the cavity combiner may be decreased to run the amplifier at a decent efficiency. The output coupling has to be adjusted.

CRISP WP 7 Page 13 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob AMPLIFIER PERFORMANCES Test conditions: Idq=2*100mA per module (nearly class B) Vds=50V SN12 is a module chosen for its average gain and efficiency. Its performances are compared with that of the whole amplifier. The RF power and drain total current of the whole amplifier have been divided by 18. The plots are quite close.

CRISP WP 7 Page 14 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob AMPLIFIER PERFORMANCES DISCREPANCIES

CRISP WP 7 Page 15 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob AMPLIFIER PERFORMANCES PULSED OPERATION UP TO 10 KW RF 100 us Vds 46V min Recorded at 5kW

CRISP WP 7 Page 16 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob FURTHER TESTS WITH 3 WINGS Check the operation with new DC distribution boards on 50Ω load and additional cooling circuit. Test with 3 adjacent wings on 50Ω load. Test with VSWR using our EH tuner.

CRISP WP 7 Page 17 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob WHAT’S NEXT? The extrusion of cooling plates has been ordered to an Italian company. The machining and electroplating of mechanical parts has been subcontracted in France. The manufacturing of the modules has been handed over to a French company. The wings will be put together by ESRF people. We launched the production of 19 (+2 spares) wings to complete the cavity combiner slots.

CRISP WP 7 Page 18 CWRF 2014 Trieste May Michel Langlois, Pierre Barbier, Jörn Jacob Thanks to my dear colleagues for their very welcomed advices Thanks to Hans Kartman (NXP) for his help in the module design You still here? Thank you for that too!