Rihua Zeng RF group, Accelerator division

Slides:



Advertisements
Similar presentations
Tom Powers Practical Aspects of SRF Cavity Testing and Operations SRF Workshop 2011 Tutorial Session.
Advertisements

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.
Lorentz force detuning measurements on the CEA cavity
LLRF Requirement and Parameters at ESS Rihua Zeng, Anders J Johansson LLRF workshop, Hamburg,
Power Requirements for High beta Elliptical Cavities Rihua Zeng Accelerator Division Lunds Kommun, Lund
RF Synchronisation Issues
European Spallation Source RF Systems Dave McGinnis RF Group Leader ESS Accelerator Division SLHiPP-1 Meeting 9-December-2011.
LLRF System for Pulsed Linacs (modeling, simulation, design and implementation) Hooman Hassanzadegan ESS, Beam Instrumentation Group 1.
RF Distribution Alternatives R.A.Yogi & FREIA group Uppsala University.
RF Cavity Simulation for SPL Simulink Model for HP-SPL Extension to LINAC4 at CERN from RF Point of View Acknowledgement: CEA team, in particular O. Piquet.
LLRF Cavity Simulation for SPL
LLRF ILC GDE Meeting Feb.6,2007 Shin Michizono LLRF - Stability requirements and proposed llrf system - Typical rf perturbations - Achieved stability at.
LLRF-05 Oct.10,20051 Digital LLRF feedback control system for the J-PARC linac Shin MICHIZONO KEK, High Energy Accelerator Research Organization (JAPAN)
1 FNAL SCRF meeting 31/10/2015 Comments from LLRF Shin Michizono (KEK) Brian Chase (FNAL) Stefan Simrock (DESY) LLRF performance under large dead time.
Recent LFD Control Results from FNAL Yuriy Pischalnikov Warren Schappert TTF/FLASH 9mA Meeting on Cavity Gradient Flatness June 01, 2010.
1Matthias LiepeAugust 2, 2007 LLRF for the ERL Matthias Liepe.
RF Development for ESS Roger Ruber and Volker Ziemann Uppsala Universitet 4 Dec Dec-20091RR+VZ: ESS RF Development.
W. 3rd SPL collaboration Meeting November 12, 20091/23 Wolfgang Hofle SPL LLRF simulations Feasibility and constraints for operation with more.
Anders Sunesson RF Group ESS Accelerator Division
RF system issues due to pulsed beam in ILC DR October 20, Belomestnykh, RF for pulsed beam ILC DR, IWLC2010 S. Belomestnykh Cornell University.
RF Cavity Simulation for SPL
Marc Ross Nick Walker Akira Yamamoto ‘Overhead and Margin’ – an attempt to set standard terminology 10 Sept 2010 Overhead and Margin 1.
Cavities Auto Recovery with Beam RF&Linac Section - ALBA Accelerators Division Francis Perez Angela Salom.
Frank Ludwig, DESY Content : 1 Stability requirements for phase and amplitude for the XFEL 2 Next LLRF system for optimized detector operation 3 Limitations.
W. 5th SPL collaboration Meeting CERN, November 25, 20101/18 reported by Wolfgang Hofle CERN BE/RF Update on RF Layout and LLRF activities for.
1 Simulation for power overhead and cavity field estimation Shin Michizono (KEK) Performance (rf power and max. cavity MV/m 24 cav. operation.
Ding Sun and David Wildman Fermilab Accelerator Advisory Committee
ESS LLRF and Beam Interaction. ESS RF system From the wall plug to the coupler Controlled over EPICS Connected to the global Machine Protection System.
John Carwardine 21 st October 2010 TTF/FLASH 9mA studies: Main studies objectives for January 2011.
R.SREEDHARAN  SOLEIL main parameters  Booster and storage ring low level RF system  New digital Booster LLRF system under development  Digital LLRF.
Thomas Jefferson National Accelerator Facility Operated by the Southeastern Universities Research Association for the U.S. Department of Energy Kirk Davis.
Preliminary Results from First Blade Tuner Tests in HTS Yuriy Pischalnikov Warren Schappert Serena Barbannoti Matteo Scorrano.
Jan Low Energy 10 Hz Operation in DRFS (Fukuda) (Fukuda) 1 Low Energy 10Hz Operation in DRFS S. Fukuda KEK.
LLRF_05 - CERN, October 10-13, 2005Institute of Electronic Systems Superconductive cavity driving with FPGA controller Tomasz Czarski Warsaw University.
Digital LLRF: ALBA and Max-IV cases RF&Linac Section - ALBA Accelerators Division Angela Salom.
Warren Schappert Yuriy Pischalnikov FNAL SRF2011, Chicago.
Overview of long pulse experiments at NML Nikolay Solyak PXIE Program Review January 16-17, PXIE Review, N.Solyak E.Harms, S. Nagaitsev, B. Chase,
Long Pulse Klystron Modulators SML (Stacked Multi-Level) topology
Matthias Liepe. Matthias Liepe – High loaded Q cavity operation at CU – TTC Topical Meeting on CW-SRF
BE-RF-FB THE LINAC4 LOW LEVEL RF 02/11/2015 LLRF15, THE LINAC4 LOW LEVEL RF2 P. Baudrenghien, J. Galindo, G. Hagmann, J. Noirjean, D. Stellfeld, D.Valuch.
1 Tuner performance with LLRF control at KEK Shin MICHIZONO (KEK) Dec.07 TTC Beijing (Michizono) S1G (RDR configuration) - Detuning monitor - Tuner control.
Aaron Farricker 107/07/2014Aaron Farricker Beam Dynamics in the ESS Linac Under the Influence of Monopole and Dipole HOMs.
Overview Step by step procedure to validate the model (slide 1 and 2) Procedure for the Ql / beam loading study (slide 3 and 4)
ESS Linac Upgrade Dave McGinnis Chief Engineer / Accelerator Division May 27, 2014.
SRF Cavities Resonance Control. CW mode of operation (FNAL’s experience). Yu. Pischalnikov W. Schappert FNAL TTC CW SRF Meeting, Cornell University, 12June,
ESS SC cavities development G. Devanz TTC meeting, march 1st 2011, Milano.
A CW Linac scheme for CLIC drive beam acceleration. Hao Zha, Alexej Grudiev 07/06/2016.
LLRF regulation of CC2 operated at 4˚K Gustavo Cancelo for the AD, TD & CD LLRF team.
ESS LLRF and Beam Interaction
Areal RF Station A. Vardanyan
ILC Power and Cooling VM Workshop
Prospects for developing new tubes
Test of the dressed spoke cavity
WP5 Elliptical cavities
Development of high-power IOTs as an efficient alternative to klystrons Morten Jensen Energy for Sustainable Science 24 October 2013, CERN.
LLRF Research and Development at STF-KEK
Overview and System Design for ESS LLRF Systems
LLRF for ESS: Requirements and System design
ILC LLRF Status Ruben Carcagno, Brian Chase
LLRF systems status update
Second SPL Collaboration Meeting, Vancouver May 2009
SPL Collaboration Meeting PAC2009
Rihua Zeng RF Group, Accelerator Division, ESS ERIC Oct 29, 2015
LLRF Functionality Stefan Simrock How to edit the title slide
CEPC RF Power Sources System
Implications of HOMs on Beam Dynamics at ESS
ATF project meeting, Feb KEK, Junji Urakawa Contents :
Managing Parameters Karin Rathsman
RF introduction Anders Sunesson RF group leader
Summary of the maximum SCRF voltage in XFEL
Presentation transcript:

Rihua Zeng RF group, Accelerator division 2015-01-13 Cavity Control, Operation, and Test Challenges at ESS and Possible Solutions Rihua Zeng RF group, Accelerator division 2015-01-13

Outline ESS Status Control, Operation, and Test Challenges at ESS Promising solutions with powerful infrastructure---MTCA system----based hardware/software/firmware Example 1: Heavy quality data Example 2: High precision RF measurement Example 3: Power overhead reduction Cavity Turn on Procedures

Accelerator Design is updating In Current Design(to date): 5 MW beam power 2 GeV protons (H+) 2.86 ms pulses 14 Hz rep rate 62.5 mA pulse current 352.21 MHz 704.42 MHz RF frequency

Target at ESS

Amplifiers/Klystron, IOT, Tetrode (2013 version, A. Sunesson) Cavity Pulse power (kW) RF Frequency (MHz) Number Sat Power (kW) Choice RFQ 1300 352.21 1 1700 Klystron Bunchers 15 2 20 SS or IOT DTL 2200 4 2900 Spoke 165-239 28 310 Tetrode Medium β 122-514 704.42 60 670 High β 394-872 120 1150 Klystron/IOT

Modulator: The Stacked Multi-Level (SML) topology (Carlos A. Martins, ESS) DC (115 kV, klystrons) (50 kV, IOT’s AC / DC DC-link 1.1 kV DC / Capacitor bank 1 kV AC 15 kHz 1 kV HF Transf. 25 kV AC + DC Filter Module #1 Module #N

IOT (Morten Jensen) Reduced velocity spread compared to klystrons (Density modulated) Biased Control Grid RF input RF output Reduced velocity spread compared to klystrons Higher efficiency No pulsed high voltage Cheaper modulator

ESS LLRF prototyping 2014-3-26, Anders J. Johansson, Lund U.

The ideal cases

Perturbations in real world Beam Loading Lorentz force detuning Microphonics Thermal effects (Quench…) Ql spread Cavity Synchronous phase Beam chopping Pulse beam transient Charge fluctuations Non-relativistic beam Pass band modes HOMs, wake-field Modulator droop and ripple Klystron nonlinearity Power Supply Reference thermal drift Master oscillator phase noise Phase reference distribution Crates power supply noise Cross talk, thermal drift Clock jitter, nonlinearity Electronics crates Further reading: LLRF Experience at TTF and Development for XFEL and ILC, S. Simrock, DESY, ILC WS 2005

Cavity Control Challenges Higher Stability requirement(±0.1 deg. ±0.1%, still in discussion with beam physics group) Long pulse(~3.5ms RF pulses) Much longer Lorentz force detuning dynamics during pulse, might not be able to get compensated by traditional way driving the piezo with a simple half-cycle sinusoid impulse Klystron output droop and ripple might be bigger due to long RF pulse High intensity (62.5mA, double than SNS) Heavy beam beam loading in cavities, require careful feedforward compensation for each beam mode during pulses, and appropriate adaptive feedforward to reduce the repetitive feedback transient response from pulse to pulse High gradient (~20MV/m, 5MV higher than SNS) 44MV/m maximum surface field(Accelerating gradient 19.9MV/m) High beam power(5MW, 5 times higher than SNS) The same situation of RF setting errors (up to 2° in phase and 2% in amplitude) might not be acceptable at ESS due to probably higher beam loss at high power linac of 5MW Spoke cavity(have not ever used in any accelerator ) Uncertainties; Energy Efficient Klystron Linearization; Minimize RF power overhead for RF control(25%10%) High availability Fast recovery from quench; Fast recovery from single/multiple LLRF, klystron, modulator, cavity, cryomodule failures 45% below saturation 54% below saturation

Control challenges: Klystron/Modulator ripples

Control challenges: Beam loading issue Normal conducting cavities (RFQ, DTL) have much lower Ql, ~ factor of 30. Control is much more difficult due to low loop gain (~2, compared to 50 in superconducting cavity) Beam loading is a very high frequency perturbations, and cannot be well compensated by integral controller from presentation of J. Galambos

Cavity Operation Challenge 155 Cavities…. Cavity gradient spread(could be up to 50%) Dynamic detuning spread Q load value spread >20% Beam velocity induced R/Q, Vc spread Synchronous phase

Operation challenges: Beam based calibration

Cavity RF/LLRF Test Challenges Test stand all over the European, but none of them in Lund(so far) How to learn as much as possible from a variety of RF tests carried out at different test stands and final accelerator tunnel, in order to better understand the cavity system and know its limitations, thereby operating the cavity system efficiently and effectively.

Advantage at ESS One cavity driven by one amplifier(klystron, IOT) for RFQ, DTL, elliptical cavities and one cavity by 2 tetrod in spoke most are cold linac high cavity bandwidth(>1kHz for SC cavity) Learn valuable experience from other labs

Advantage of new technology Powerful new technology: MTCA system Powerful hardware performance: 10 input channel (2.5 times as SNS ), ~1000 times bigger memory in FPGA, faster CPU, communication, higher SNR>70dB Memory resolution able to <10ns We should really aware the transformation such new technology could bring, and how to best apply in ESS, make full use of such a technology

Addressing beam loading issue Feed forward table adjustable resolution (better performance when resolution <100ns. Beam loading FF compensation

We should really aware the transformation such new technology(MTCA) could bring, and how to be best applied in ESS, make full use of such a technology We could change the way doing things, with such powerful technology and advantages at ESS But it is only happen if we can fully understand such system and appreciate the beauty it brings

Example 1: See in depth: Higher quality data higher resolution, adequate data sets, higher SNR Be able to carry out elaborate experimentation and obtain required data for particular purpose Real time measurement

See in depth: Higher Resolution data Beam loading: What happens during 1us 52.7kV (0.29% of operating voltage 18MV) for the 1μs-long beam pulse induced voltage Crucial limitation

Powreful technology: Higher resolution data What happens in 100ns(3MHz bandwidth system)

Powreful technology: High Signal to Noise Ratio(SNR) SNR 75dB from IQ detection: 70dB SNR cause more than 6% power overhead, while 75dB ~3%; 75dB possible?

Get data as we required With high performance hardware, we are able to carry out elaborate experimentation and obtain required data for particular purpose Example: Lorentz Force Detuning Compensation Static LFD coefficients Dynamic LFD spectrum Time domain piezo tuner transfer function(pulse mode, impulse response)

Well-Recorded data in high details Motor tuner transfer function/DESY Quench limitation identification/DESY Klystron input-output characteristics/JPARC Lorentz force detuning/Fermilab

Example 2: High precision RF measurement for basic cavity parameters Ql Dynamic detuning R/Q Phase Amplitude

High precision RF measurement: Ql, detuning

High precision RF measurement: R/Q Calibration

Beam based calibration: Phase&Amplitude

There is more…

Natural way to calibrate system parameters Focus on converging the model to the “true” system Produce output by model predicting/theoretical calculation Measure output by doing specific testing Least-square methods to identify systematic errors Least-square methods to modify model parameters so as to converge to “true” system

However, There no absolute “true” system, no absolute “true” data, even no “true” parameters(voltage and phase of the cavity?) In reality, it is less important to identify the true system, but more important to identify a good input-output description of the system

So can we accept a “modified” model having robust/best averaging/or simply constant prediction errors, comparing with measured data? And use this “modified” model to generate ”modified” parameters, to configure, control, operate the system? And do it in automatically way?

Example We accept accelerating voltage Vc, synchronous phase φb, ±1%, ±2%, or even more, with “true” values. And derive new R/Q*, Ql*, Δω*, aslo t_inj, pre-detuning in model, by referring this voltage, and phase, even if these new generated value different from designed/measured R/Q, Ql, Δω. A robust model best describing system then is obtained, even if have discrepancy with designed/measured one, as long as the discrepancy is robust and we can control.

If there is voltage setting errors, but we still accept it as “correct” value in model, and just change R/Q to R/Q* in FF table, to make cavity gradient reach the same level. The R/Q* will be default value. It will lead changed t_inj, predtuning, and possible other parameter not identical with design value, but that doesn’t matter, since we really care is to maintain constant field.

Example 3: Power overhead reduction----running close to saturation

Overhead at beam commissioning Behaviors are different among different beam modes peak power depends on the error when system transient response reaches its first overshoot peak, limited by system bandwidth.

Promising consequence Doing thing in a simple, straightforward way: Measured dynamic detuning

Others Cavity gradient spread(can be up to ±30%) Ql spread ( can be up to ±20%) Spoke cavity Allowable for several cavities failure, fast recovery Work and change quickly at different gradient, phase

It is in an early stage, but have quite tough schedule.. It is a iterative process. Keep learning, and keep upgrade. The requirement & functionalities would change, as we get more and more understanding the hardware/software/firmware need more input (theoretical analysis, calculation and simulation, and practical test and knowledge, expertises) From test, measurement, To decide what is necessary and practical to implement(drift beam calibration? beam based feedback? on-line cavity model? more measurement input? High accuracy? More data?)

Thanks!