Upgrades and EM simulations for the Diamond SR HP Amplifiers

Slides:



Advertisements
Similar presentations
IOT Measurements & Amplifier Improvements at Diamond
Advertisements

Tom Powers Practical Aspects of SRF Cavity Testing and Operations SRF Workshop 2011 Tutorial Session.
11/27/2007ILC Power and Cooling VM Workshop Mike Neubauer 1 RF Power and Cooling Requirements Overview from “Main Linac Power and Cooling Information”
30 th September 2004 High Power RF Couplers James Rogers High Power RF Couplers ELSRF Daresbury Laboratory.
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,
RF Safety Discussion Derun Li/Bob Rimmer Center for Beam Physics Lawrence Berkeley National Laboratory SRF Institute, JLab.
1 Operating Experience and Reliability Update on the 5 kW CW Klystrons at Jefferson Lab Richard Walker & Richard Nelson Jefferson Lab, Newport News VA.
Injector RF Design Review November 3, 2004 John Schmerge, SLAC LCLS RF Gun Thermal Analysis John Schmerge, SLAC November 3,
Safety Review: RF Issues Derun Li Absorber Safety Review December 9-10, 2003 Lawrence Berkeley National Laboratory Berkeley, CA
RF Stability Working Group Jorn Jacob (ESRF), John Byrd (LBNL) General Issues RF phase and amplitude noise –filtered by cavity and translate into timing.
Proton Source Workshop December 7 & 8, 2010 John Reid December 8, 2010.
Digital measurement system for the LHC klystron high voltage modulator D. Valuch, A. Mikkelsen, G. Ravida, O. Brunner.
Confidential / Property of Danfoss Drives A/S DKDD-SMC 1 Drives Division Danfoss presents - VLT ® 2800 Series.
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 !
Linac Marx Modulator Update Trevor Butler 5/20/2015.
Accelerators for ADS March 2014 CERN Approach for a reliable cryogenic system T. Junquera (ACS) *Work supported by the EU, FP7 MAX contract number.
Clustered Surface RF Production Scheme Chris Adolphsen Chris Nantista SLAC.
1 ELE5 COMMUNICATIONS SYSTEMS REVISION NOTES. 2 Generalised System.
CRYOGENICS FOR MLC Cryogenic Piping in the Module Eric Smith External Review of MLC October 03, October 2012Cryogenics for MLC1.
Neutrino Factory Workshop, IOP, 28th October 2003 RF Systems David M Wilcox.
RF Development for ESS Roger Ruber and Volker Ziemann Uppsala Universitet 4 Dec Dec-20091RR+VZ: ESS RF Development.
Andrew Moss ASTeC CM32 9t h February 2012 RAL MICE RF System.
Operational experience of high-power RF at Diamond Light Source Chris Christou, Pengda Gu, Alun Watkins Diamond Light Source.
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,
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.
Commissioning of the ALBA IOT-Transmitters Paco Sanchez - 14th ESLS RF - ELETTRA, September Paco Sanchez, RF Group, CELLS (Consortium for.
Network Media. Copper, Optical, Fibre (Physical Layer Technologies) Introduction to Computer Networking.
ALBA RF Amplifiers based on IOTs CWRF08 - CERN, March 2008 Michel Langlois & Paco Sanchez 1 Michel Langlois & Paco Sanchez.
Operational experience of high-power RF at Diamond Light Source
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.
Solid State Amplifier Circuit Design Student: Branko Popovic Advisor: Geoff Waldschmidt.
13 th ESLS RF Meeting – 1 st October 2008 DAMPY Cavity 1/20 80 kW at Dampy Francis Perez.
Power Electronics and Switch Mode Power Supply
Diamond LLRF Activities Pengda Gu For DLS RF Group.
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.
PS-ESS and LEBT State of the art Lorenzo Neri Istituto Nazionale di Fisica Nucleare Laboratori Nazionali del Sud.
ALBA RF Systems Francis Perez.
Long Pulse Klystron Modulators SML (Stacked Multi-Level) topology
Status of the Diamond Storage Ring RF Systems Morten Jensen on behalf of Diamond Storage Ring RF Group ESLS RF 2009.
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.
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.
RFQ coupler S. Kazakov 07/28/2015. Requirements: Coupler requirements Expected problems: Heating (loop, ceramic window, etc.) Multipactor Solutions: Appropriate.
Linac RF System Design Options Y. Kang RAD/SNS/NScD/ORNL Project – X Collaboration Meeting April , 2011.
Improvements to Diamond Light Source RF Amplifiers Peter Marten On behalf of the Diamond RF Group* *also C. Christou, P. Gu, M. Maddock, S. A. Pande, A.
Areal RF Station A. Vardanyan
ILC Power and Cooling VM Workshop
Storage Ring RF Systems
Overview of cavity reliability at Diamond Light Source
Status of RF at Diamond Light Source and overview of upgrade plans
TTC Topical Workshop - CW SRF, Cornell 12th – 14th June 2013
An X-band system for phase space linearisation on CLARA
Developments of High CW RF Power Solid State Amplifiers at SOLEIL
BCTW calibration status and future
RF operation of REX-ISOLDE
Test plan of ESS HB elliptical cavity
Jefferson Lab Low Level RF Controls
CEPC RF Power Sources System
COOLING OF POWER DEVICES
First High Power Test of the ESS Double Spoke Cavity package
RF systems introduction
Physics Design on Injector I
Status and New Developments of ALBA RF Systems
Status and New Developments of ALBA RF Systems
Breakout Session SC3 – Undulator
IOT operation in the SPS Long term experience TWC 800 MHz
Presentation transcript:

Upgrades and EM simulations for the Diamond SR HP Amplifiers Morten Jensen on behalf of the SR RF Group CW and High Average Power Workshop 2012 - BNL

SR RF Systems RFTF Cryogenic Plant HV PSU Circulator and load IOTs and Combiner Cryogenic Plant LLRF , DAs and Aux Supplies Superconducting Cavities

Most upgrades driven by need to improve reliability Main issues: Cavity failure Frequent cavity trips Early IOT failure rate Spurious arc Increasing beam current RF MTBF Early years: MTBF: ~ 40 hrs 2012 (year to date) > 335 hrs

12 IOT failures: Average filament hours on failure: 4500 New Tender: Change of IOTs Original IOT: TH793 (TED) 12 IOT failures: Average filament hours on failure: 4500 New Tender: IOTD2130 (E2V) or TH793-1 (new TED IOT) TH793 IOTD2130 Main differences: Single output cavity No body current connection Modified cooling circuit Tuning and installation Circuit dimensions

ARC Detector modifications Suspected false trips from Waveguide Circulator and RF Load arc detectors. Confirmed susceptibility to false trips: Mains cable PCB EMI Excessive circuit gain Solution: Reduced Sensitivity Gain: 10M → 200k Energy for trigger: 1 – 2 J No more trips Trigger caused by mobile phone Arc detector output Output from front end

Spark Box In-house design and build Output voltage can be changed by adjusting the spark gap The spark energy is determined by the number of HV capacitors linked together Output of original arc detector saturates even with very weak sparks. A gain of 10k is enough to detect sparks of 0.1 Joule energy ARC detector Optical fibre Capacitor mounting plate Adjustable Spark gap Safety shorting bar

Investigation of IOT failure revealed Blackened collector Glycol Change Investigation of IOT failure revealed Blackened collector Diamond IOT after 1300 hrs Broadcast IOT with 8 years service Cause: Suspected lack of cooling Chemical change to Glycol used introduced Silicone. Silicone prevents wetting of collector surface reducing cooling. Chemical analysis of alternative glycols Heated detergent wash prior to glycol change New glycol mix in operation DowCal10 changed for ThermoCal

NI PXI Data Acquisition 100 S/s to ~800 kS/s Temperature, V, I, R 8 channel, 60 MS/s 12bit, 128M Speed Examples Hardware Very Slow < 10 Hz EPICS PVs VME / IOC Slow 10–100 Hz Temperatures Cryogenics NI Compact RIO Fast 100 Hz -800 kHz Vacuum Analogue voltage / current Very fast ≤ 60 MHz Cavity voltage RF power etc PXI Scope Cards RF Waveforms 500 MHz waveforms Pulses and fast rise times Typical oscilloscope ≥ 1 GHz plus 3 off G64 Canberra X-ray monitors ION Chamber based monitoring One installed per cavity

Master Oscillator Modification IFR (Aeroflex) 2040 Phase glitches observed when communicating with MO GPIB interface located on 5 Volt PCB supply track. Current pulse causes voltage drop (0.0008 V) producing noise. Before After In house investigation: Circuits modified to supply GPIB circuitry directly from PSU and with additional decoupling capacitors.

Fast IOT Fault Detection and Isolation Purpose IOT breakdown is single largest amplifier fault Fault on one IOT isolates HV for all 4 IOTs Typically 10-15 trips per year (6 in 2011) 8 IOTs in operation Recovery is fast – but beam is lost Possible solution Detect IOT fault (µs) Isolate IOT HV (dissipated energy < 9J) Maintain beam –> Other IOTs to ramp up Re-instate IOT -> Other IOTs ramps down

Successful First Test of Principle Fast IOT Fault Detection and Isolation Successful First Test of Principle Close up of IOT turn OFF and ON Small voltage disturbance during switching Cavity 1 Voltage Cavity voltage Forward Power Beam current = 210 mA Reflected Power IOT 2, 3, 4 IOT 1 OFF IOT 1 IOTs 2, 3 and 4 UP IOT power Note IOT 1 turned off and IOTs 2,3 and 4 compensate 20 ms Preparation: Quench Detector turned OFF Reflected power trip turned off Further work needed to maintain beam at high power operation

RF Test Facility Shielded high power cavity conditioning area Full PSS control 300 kW RF power from any of the 3 amplifiers Integration into the Liquid Helium Refrigerator Full cavity control system

The Reject Loads The present load uses a mixture of 40% Glycol and 60% Water – Glycol to be eliminated. The new load will use pure water – required for IOTs Design Goal Co-axial 6-1/8” line size; modification of existing loads Well matched to the input transmission line S11 < -30dB @499.654 ± 2 MHz Able to handle 80 kW

Dielectric Properties of Water & Glycol 40% Glycol-Water Mixture @25C Pure Water @25C Dielectric Constant () 56 78 Loss Tangent (tand) ~0.2 ~0.024 Glycol-Water Mixture Impedance matching is easier for short loads Very good absorber of RF Power  Fast attenuation leading to compact design Water Impedance matching is relatively difficult Not very good absorber of RF power (vs Glycol- Water mixture)  Slow attenuation leading to larger length Technique of Microwave Measurements edited by C G Montgomery, Rad. Lab. Series Vol. 11

The High Power Co-axial Load Extra length to absorb remaining energy Enlarged Section at A-A Impedance matching section PTFE Water Cu D d d1 er=2.1 er=78 A Input A New Water Water PTFE Air 960 mm - Length of existing load Diameters and lengths of the PTFE cylinders are changed in steps for impedance mathcing and to reduce power density

Comparison of match of original load to new design New design with demin water -30 dB for 500 MHz +/- 2 MHz Existing design with 40% glycol Improved match at 500 MHz but narrow band

Power loss density along the length Low electric field strength → low risk of breakdown Water flow rate of 70 l/min → acceptable delta T Power loss density RF Further work to include: Tolerance analysis Variation in match with water temperature Mechanical design Build of Prototype

Optimisation of 3-Stub Tuner To match the cavities when operated at non-optimum conditions → Higher / Lower Qext Experimental optimisation: Takes too long due to long time constants 24-48 hrs Reduced risk due to high electric field regions Minimization of critical thermal loads and mechanical fatique CAVITY-1 Total length of waveguide = 13215.9 mm Guide wavelength = 795.1 mm Total length/ lg = 16.6217 Length of Equivalent Waveguide = 0.6217* lg = 494.3 mm Tuner 1 2 3 Equivalent Waveguide 3 Stub Tuner

Optimisation of 3-Stub Tuner Comparison between simulation and measurement Surface power loss density W/m2 Hotspots indicate regions with high heat loads

On behalf of the RF Group Morten Jensen Pengda Gu Matt Maddock Peter Marten Shivaji Pande Simon Rains Adam Rankin David Spink Alun Watkins Thank you for your attention