Raja Ramanna Centre for Advanced Technology

Slides:



Advertisements
Similar presentations
Overview of SMTF RF Systems Brian Chase. Overview Scope of RF Systems RF & LLRF Collaboration LLRF Specifications for SMTF Progress So Far Status of progress.
Advertisements

Lorentz force detuning measurements on the CEA cavity
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,
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
Raja Ramanna Centre for Advanced Technology
Components & Subsystems New generations of RF Amplifiers : from system requirements to technologies Michel Caplot, Christian Robert, Michel Grezaud, Bernard.
POWER PLANT USED IN TELECOM
Conventional Tubes Conventional Device tubes cannot be used for frequencies above 100MHz 1. Interelectrode capacitance 2. Lead Inductance effect 3. Transit.
New Electron Beam Test Facility EBTF at Daresbury Laboratory B.L. Militsyn on behalf of the ASTeC team Accelerator Science and Technology Centre Science.
CommunicationElectronics Principles & Applications Third Edition Chapter 6 Radio Transmitters ©2001 Glencoe/McGraw-Hill Louis E. Frenzel.
1Matthias LiepeAugust 2, 2007 LLRF for the ERL Matthias Liepe.
PROTON LINAC FOR INDIAN SNS Vinod Bharadwaj, SLAC (reporting for the Indian SNS Design Team)
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.
CLIC Workshop, February, CERN. I. Syratchev Roadmap for CLIC high-efficiency klystron development I. Syratchev, CERN.
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.
Status of the 1.2 MW MB-IOT for ESS Morten Jensen CLIC Workshop 2016, January, CERN.
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
ALBA RF Systems Francis Perez.
RF Power for VTS & HTS Purushottam Shrivastava, P. Mohania, D. Baxy, V. Rajput PHPMS Raja Ramanna Centre for Advanced Technology, Indore October 28, 2010.
IIFC Meeting February 24-25, 2015, RRCAT P. R. Hannurkar, Akhilesh Jain, M. R. Lad RF Systems Division 650 MHz RF Power 1.
New prototype modulator for the European XFEL Project (DESY) Pulse Step Modulator (PSM) Technology for long pulse applications.
Project X High Power 325 MHz RF Distribution and Control Alfred Moretti, Nov 12, 2007 Project X Workshop.
Status of Vertical Test Stand at RRCAT P Shrivastava, P Mohania,D.Baxy, Vikas Rajput S C Joshi, S Raghavendra,S K Suhane RRCAT, Indore November 26, 2012.
The Working Theory of an RC Coupled Amplifier in Electronics.
Heung-Sik Kang Pohang Accelerator Laboratory
High-efficiency L-band klystron development for the CLIC Drive Beam High-efficiency L-band klystron development for the CLIC Drive Beam CLIC workshop,
Linac RF System Design Options Y. Kang RAD/SNS/NScD/ORNL Project – X Collaboration Meeting April , 2011.
Status and plans of drive beam components and tests Status and plans of drive beam components and tests CLIC review, March 1 st, 2016Steffen Döbert, BE-RF.
FUNCTION GENERATOR.
High Power RF Systems for 2-8 GeV Fast Cycling Synchrotron PROJECT X (ICD-2) John Reid September 11, 2009.
Status of the sub-harmonic bunching system for the CLIC DB injector front end Hamed Shaker School of Particles and Accelerators, Institute for Research.
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
PADME Front-End Electronics
Results of on-site performance tests on 20kW Solid State Wide Band Amplifier for the CLIC DB Front End at CERN* Purushottam Shrivastava, P. Mohania,
Prospects for developing new tubes
Multi-stage pulse compressor
Communication 40 GHz Anurag Nigam.
How does a klystron work? TE-MPE Section Meeting Karolina Kulesz
High efficiency work and MBK development for accelerators
Development of high-power IOTs as an efficient alternative to klystrons Morten Jensen Energy for Sustainable Science 24 October 2013, CERN.
Visit for more Learning Resources
CLIC DB injector front end update on the work package
Development of X-band 50MW klystron in BVERI
An X-band system for phase space linearisation on CLARA
Status of the CLIC main beam injectors
Developments of High CW RF Power Solid State Amplifiers at SOLEIL
BE/RF-IS Contribution to LIU C. Rossi and M. Paoluzzi
Wideband, solid-state driven RF systems for PSB and PS longitudinal damper.
10 MHz amplifier status G. Favia
Application of the moderate peak power (6 MW) X-band klystron’s cluster for the CLIC accelerating structures testing program. I. Syratchev.
WP11: electron and proton beam testing
Notkestrasse 85, Hamburg, Germany
X-band Facilities and High Gradient Tests Stands Around the World
High Efficiency X-band Klystron Design Study
Measurements, ideas, curiosities
Accelerator Layout and Parameters
CW Operation of XFEL Modules
CEPC RF Power Sources System
BESIII EMC electronics
Status of the CLIC Injector studies
RF Pulse Shaping.
CLIC Feasibility Demonstration at CTF3
Presentation transcript:

Raja Ramanna Centre for Advanced Technology Design, Development and test results of 20kW, 499.75 MHz Solid State Wide Band RF Power Amplifiers for the CLIC injector pre-buncher * Purushottam Shrivastava, P. Mohania, A. Mahawar, P.D. Gupta Raja Ramanna Centre for Advanced Technology Indore, India CLIC Workshop Jan 18-22, 2016 * DAE (India) CERN Collaboration under NAT Protocol

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN Motivation Under DAE (India) CERN collaboration in Novel Accelerator Technologies, of which CLIC collaboration is a part, a 20kW Solid State RF Power Amplifier R, D & D effort by RRCAT, Indore was agreed an as R & D and protyping in this state of the art area. RRCAT had earlier built a 476 MHz, 10kW Solid State RF Power Amplifier for use in its FEL projects. RRCAT has also built solid state RF systems for the characterization of Superconducting cavities at 325 MHz, 650MHz, 1.3 GHz. In order to achieve the desired specifications and feasibility RRCAT first developed 1kW, 5 kW intermediate SSPA stages as a part of development and improvements/ modifications were incorporated for realising the final 20kW power level. In earlier workshop we reported a prototype 5kW SSPA development which served as a base for development of present wide band 20kW SSPA. We have developed the complete amplifier in-house using the design, fabrication, testing and qualification facilities available at RRCAT. Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN Outline Technical requirements & Specifications of the 20kW SSPA Device selection and amplifier design 20kW SSPA architecture 5kW prototype development for feasibility and performance characteristics studies Final amplifier development Test results Conclusion Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Modulator-klystrons, 1 GHz, 15 MW CLIC DB front end Gun SHB 1-2-3 PB Buncher Acc. Structures IOTs ?, SSPA 500 MHz Modulator-klystrons, 1 GHz, 15 MW ~ 140 keV ~ 12 MeV Diagnostics ~ 3 MeV For time being only major component development: GUN, SHB, high bandwidth 500 MHz source, 1 GHZ MBK, modulator and accelerating structure in an high power test stand Courtesy: Steffen Doebert

Sub-harmonic bunching system Status: RF design existing, mechanical design done, Discussion with CERN work shop on realization Power source: 500 MHz, 20-115 kW, wide band (60 MHz) sources needed for fast phase switching. Solid state favored Comment: On 20kW prototype Done under collaboration with RRCAT SHB 1 SHB 2 SHB 3 Beam velocity 0.62 c Current 5 A Voltage 15 kV 30 kV 45 kV Bunch form factor 0.058 0.57 0.73 Detuning 1.6 MHz 12.1 MHz 12.7 MHz Hamed Shaker Courtesy: Steffen Doebert

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN Compact, 10kW solid state RF power amplifiers, @476 MHz using LDMOS transistors and novel planar combiners and dividers for pre-buncher cavity of injector LINAC for CUTE FEL and IR-FEL project at RRCAT 10kW SSPA during tests A compact 10 kW, 476 MHz solid state radio frequency amplifier for pre-buncher cavity of free electron laser injector linear accelerator. Published in: Review of Scientific Instruments (Volume:84 , Issue: 9 ) Sept 2013. Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Phase variation shot to shot, flat top Specifications of the 20kW Solid State Amplifier Parameter Nominal value Unit Output power 20 kW Frequency 499.75 MHz Band width (3dB) 58 Pulse Length 140.3 micro sec Repetition rate 50 Hz Phase variation shot to shot, flat top ~1 deg Amplitude stability % Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN RF Power LDMOS Transistors Rugged N—Channel Enhancement--Mode Lateral MOSFETs Withstands high VSWR industrial (including laser and plasma exciters), broadcast (analog and digital), aerospace and radio/land mobile applications. • Unmatched Input and Output Allowing Wide Frequency Range Utilization 1.8 and 600 MHz,1250 W CW, 50 V • Single--Ended or in a Push--Pull Configuration • Qualified Up to a Maximum of 50 VDD Operation • Characterized from 30 V to 50 V for Extended Power Range • Suitable for Linear Application with Appropriate Biasing • Integrated ESD Protection with Greater Negative Gate--Source Voltage Range for Improved Class C Operation • Characterized with Series Equivalent Large--Signal Impedance Parameters Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Salient Features of 20kW SSPA Developed using high power push-pull LDMOS transistors The push-pull devices are operated under single ended configuration to reduce space and improve repeatability. The same design has been used to develop two 10 kW SSPA at 476 MHz for injector LINACs of CUTE FEL and Indus synchrotrons. The 20 kW is achieved by combination of 32 transistors. The high power combination is achieved using microstrip line planar combiner (Wilkinson Type). Design is highly modular, and size of each amplifier pallet (one transistor based amplifier), is 5cmx10cm only. A single pallet can provide upto 1400W peak power.

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN 5kW Amplifier Module 210mmx300mm Test results of the 5kW prototype amplifier Parameter Test Result Comments Peak Power obtained 67.1dBm (~5120W) The maximum input power required is +13dBm. Gain @ 5kW 57 dB 54dB @499.75MHz @469.75MHz @529.75MHz Bandwidth (3dB) 60 MHz (+/-30MHz) Centre Frequency 499.75MHz Pulse To Pulse Amplitude variation ~0.1dB @67.1dBm Pulse to Pulse Phase variation ~1° In pulse amplitude variation <0.2dB @ 67.1dBm In pulse phase variation <2° Amplifier Module enclosed and mounted on heat sink Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Test Results of the 5kW prototype SSPA module Test conditions: 50Hz repetition rate, 150µs pulse width, Input Power, 12.5dBm Output Power vs Frequency response. Gain characteristics at 499.75 Mhz Gain characteristics at 470.75 Mhz Gain characteristics at 528..75 Mhz Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN 5kW Wideband SSPA Delivery to CERN from RRCAT 5kW prototype SSPA received at CERN undergoing tests during August 2015 Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Amplifier design The amplifier is developed using eight amplifier modules capable of providing up to 4 kW of pulse power, which are combined by planar Wilkinson combiner and divider to generate 20 kW of pulsed output.

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN Description of stages of amplifier The amplifier has been developed as a three stage amplifier which consists of the following stages. 1 W Pre-driver amplifier 100 W GaN HEMT based driver amplifier 4kW High Power stage which is developed by combining 4 LDMOS transistors using Wilkinson combiner and divider networks on low loss flexible PTFE based laminates. 8 units of 4kW modules combined to provide over 20kW output. The switching ON time is defined by a RF switch which is having a controlled mono-shot circuit which sends TTL signal to switch for 150µs at rising edge of the input trigger (delay in RF ON ~200ns) The three stages of the amplifier uses the following power supplies 1. 1W Pre-driver amplifier 24V, 600mA 2. Driver Amplifier 32V, 200mA for drain and -3.15V for Bias 3. High power stage 55V, 2A for drain and 2.15V for Bias Input trigger signal 2.5V-5 V, 2 µs (high Impedance) Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

4kW module with 8:1 micro-strip power combiner 4kW amplifier modules High Power Microwave combiner (microstrip line based) 8:1

20kW pulsed Wide band solid state Peak Power @ 499.75MHz ≥ 73.0dBm Gain @Peak Power (499.75 MHz) 59 dB 3 dB bandwidth @14dBm Input 470.75 MHz- 528.75 MHz Pulse width (user settable) up to 140.3 µs PRR up to 50 Hz Input Connector Type-N (F) Output Connector DIN 7/16 (F) Pulse to pulse variation in amplitude < 0.1dB Pulse to pulse variation in phase < 1°

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN 20 kW SSPA Cabinet Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Details of the Front Panel Controls Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN 7/16 DIN ( Deutsches Institut für Normung) output connector of SSPA Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN Tests done on the 20kW SSPA at RRCAT, Indore, India Heat run tests conducted in lab environment with temperature around 25°C. The amplifier takes half an hour to reach thermal equilibrium, the amplifier power reduced by around 0.2dB from cold condition to thermal equilibrium and afterwards it remains consistent. The pre-driver, driver, all the eight amplifier modules and the complete amplifier system were characterized. The characterization was done using a signal generator in pulsed mode with pulse width 140.3μs and duty cycle 50 Hz. Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Amplifier amplitude and phase response The subsequent images shows the amplitude and phase response of the output pulse power at different frequencies across the frequency band. The amplitude shape is obtained by using a Peak Power analyzer and the phase response is obtained using a phase detector card. Test conditions: 50 Hz repetition rate, 140.3 μs pulse width, Input Power 14 dBm; Phase card response: 10 mV/degree Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Phase and amplitude response at 470.75 MHz Picture on left is the output of the phase card which shows the variation of the output power phase with respect to input during pulse. The right image is of detected power at peak power analyzer. The phase card response is 10mV/degree. The two markers are set at 40 μs and 130 μs in the lower image. The phase variation in pulse is 1.5 degree and amplitude variation ~0.2dB. Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Phase and amplitude response at 499.75 MHz The picture on left is the output of the phase card which shows the variation of the output power phase with respect to input during pulse. The right image is of detected power at peak power analyzer. The phase card response is 10mV/degree. The two markers are set at 40 µs and 130 µs in the lower image. The phase variation in pulse is 3.3 degree and amplitude variation ~0.2dB. Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Phase and amplitude response at 528.75 MHz the picture left above is the output of the phase card which shows the variation of the output power phase with respect to input during pulse. The image on right is of detected power at peak power analyzer. The phase card response is 10mV/degree. The two markers are set at 40 μs and 130 μs in the lower image. The phase variation in pulse is 1.5 degree and amplitude variation ~0.2dB. Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN Conclusion: The complete 20kW wide band SSPA has been designed, developed and subjected to long duration endurance testing at RRCAT, Indore. Amplifier power reaches thermal equilibrium after 30 minutes and has excellent phase and amplitude stability meeting specifications. 4 channel D. C. power supply which has stability of better than +/-0.05% have been used as bias supplies. The desired specifications have been achieved and scope for further improvements/upgrades depending upon application in the buncher can be taken up as per feedback from the users. The 20kW SSPA has been delivered to CERN. Some misalignments in the box and RF routing during transportation is being corrected after which the final tests will be repeated at CERN. Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN

Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN THANK YOU Purushottam Shrivastava, RRCAT: CLIC WS Jan 18-22, 2016 CERN