T24 results and comparison to the preceding studies on CLIC prototype structures May 17, 2011 T. Higo (KEK)

Slides:



Advertisements
Similar presentations
Breakdown Rate Dependence on Gradient and Pulse Heating in Single Cell Cavities and TD18 Faya Wang, Chris Nantista and Chris Adolphsen May 1, 2010.
Advertisements

CERN-KEK X-band collaboration 3 Dec T. Higo on behalf of X-band group of KEK.
High gradient studies in simple setups (for discussion) T. Higo.
Report from KEK High gradient study results from Nextef (+ other related activities) LCWS2011, Granada Sep. 27, 2011 T. Higo.
Status of KEK production July 11, 2008 at SLAC KEK T. Higo et al., Accelerator div. T. Takatomi et al., Mech. Eng. Center.
X-band Structures Test Results at NLCTA Faya Wang Chris Adolphsen, Christopher Nantista 9-Feb-11.
High gradient features from Nextef on recent CLIC prototype structures US-HG workshop, SLAC 9 February 2011 T. Higo representing X-band group of KEK.
Experimental breakdown studies – breakdown diagnostics Linking simulation and experiment Jan W. Kovermann, CERN, RWTH Aachen SLAC workshop July 2009.
Dark current measurement at KEK M. Gerbaux, S. Döbert, T. Higo, S. Matsumoto, K. Yokoyama.
1 More on gas filled rf cavities Alvin Tollestrup RF One Day Workshop Oct 15, 2008.
First approach to the SuperB Rings M. Biagini, LNF-INFN April 26th, 2006 UK SuperB Meeting, Daresbury.
1 X-band Single Cell and T18_SLAC_2 Test Results at NLCTA Faya Wang Chris Adolphsen Jul
Report from Nextef IWLC10, Genève, Oct. 20 T. Higo (KEK)
RF BD statistics in the TD26CC accelerating structure J. Giner-Navarro 18/11/2014 CLIC Breakdown meeting 118/11/2014J. Giner-Navarro.
Results from Nextef Observations in high gradient tests of CLIC Prototype Structures and associated study activities CLIC2013, CERN 29 January, 2013 T.
KEK activities on CLIC X-band Accelerating Structures Tsinghua Univ., March 24 T. Higo (KEK)
Accelerating structure test results and what’s next Walter Wuensch CTF3 collaboration meeting
R&D status and future strategy in KEK X-band area May 16, 2011 T. Higo (KEK)
Update of KEK X-band Research Activity March 3, 2009 Shuji Matsumoto Accelerator Laboratory, KEK 2009/3/31US High Gradient Workshop.
日米協力 US/Japan cooperation Research of High Gradient Acceleration Technology for Future Accelerators progress report New proposal 7.
Statistical analysis of RF conditioning and breakdowns Jorge GINER NAVARRO CLIC Workshop /01/2015 J. Giner Navarro - CLIC WS20151.
Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann
CLIC Workshop – CERN, October / 17 DC breakdown experiments for CLIC CERN, TS-MME Antoine Descoeudres, Trond Ramsvik, Sergio Calatroni, Mauro Taborelli.
Recent High-gradient test result at KEK Linear Collider Workshop 2012 Arlington, Texas (WebEx) 25 October, 2012 Toshi Higo and X-band group of KEK.
L-band (1.3 GHz) 5-Cell SW Cavity High Power Test Results Faya Wang, Chris Adolphsen SLAC National Accelerator Laboratory
Performance of CLIC prototype accelerator structures tested at Nextef CLIC February 2014 Toshiyasu Higo (KEK)
High Power Test of Mizuno - Ohtsuka Dry Load S. Matsumoto and T. Higo Report made on
Summary of progress towards CLIC goals and next steps for structure testing 6 th X-band collaboration workshop, April 18 th- 20 th 2012 Steffen Döbert,
A Study of RF breakdown of Narrow Wave Guide Shuji Matsumoto Kazue Yokoyama Toshi Higo Accelerator Lab., KEK 2016/1/41SLAC Workshop 8-10 July 2009.
KEK workshopWalter Wuensch18 April 2012 Status and objectives of the CLIC X-band and high- gradient activity.
High gradient study at KEK CLIC08, Oct , 2008 T. Higo.
PETS TESTING ANALYSIS 4 th X-band Structure Collaboration Meeting 3 rd May 2010 Alessandro Cappelletti for CLIC collaboration.
Progress of X-Band Accelerating Structures LINAC10, Tsukuba 17 Sep T. Higo (KEK)
Status report from KEK Feb. 26, 2010 T. Higo, S. Matsumoto T. Takatomi, Y. Higashi and X-band group.
Nextef results CLIC09, Oct T. Higo (KEK). Contents Quadrant high gradient test status – Initial processing and power limit – VAC characteristics.
TD18 High Power Test Results Faya Wang Chris Adolphsen May 3, 2010.
W. Wuensch CLIC project meeting High-power rf structure testing.
Status of high gradient experiments at Nextef Kazue Yokoyama, Toshiyasu Higo, Yasuo Higashi, Shuji Matsumoto, Shigeki Fukuda Accelerator Laboratory, KEK.
Nextef results & status International Workshop on Breakdown Science and High Gradient Technology KEK, Japan 18 April 2012 Toshi Higo.
Breakdown statistics in the large- electrode DC spark system Anders Korsbäck, BE-RF-LRF University of Helsinki Special thanks to Walter Wuensch and Jorge.
Review of the rf working group of the ICFA Mini Workshop on Novel Accelerators and Colliders which was associated with the Bob Siemann Memorial Symposium.
Discussion on critical issues for testing: breakdown identification, preparation for test, processing protocol, etc. 4 th Annual X-band Structure Collaboration.
Some information from Nextef For poster session in IWLC T. Higo.
Accelerating structure prototypes for 2011 (proposal) A.Grudiev 6/07/11.
Update on PETS experiments (Igor for the CLIC collaboration)
Nextef status and expansion plans Shuji Matsumoto for KEK Nextef Group /5/51 4th X-band Structure Collaboration Meeting, CERN.
High Power Crab Cavity Testing Ben Woolley HG2016 Argonne National Lab. 8 th June 2016.
Test Accelerating Structures Designs, Objectives and Critical Issues
KEK Status and plans of structure production and testing
Breakdown position analysis
SOME MORE STATISTICAL ANALYSIS OF TRAINING DATA
Electrical Properties of MPPC/SiPM/GMAPD’s
Project Controls: As-Built S-Curves
Effort to identify the critical issues for high gradient
Application of the moderate peak power (6 MW) X-band klystron’s cluster for the CLIC accelerating structures testing program. I. Syratchev.
Review of rf structure test results
Breakdown meeting Noora-Mari Pienimäki
Recent high-gradient testing results from the CLIC XBoxes
High Gradient tests at the KEK Nextef Facility
A Study of RF breakdown of Narrow Wave Guide
NanoBPM Status and Multibunch Mark Slater, Cambridge University
Progress in the design of a damped an
5th X-Band Structure Collaboration Meeting
Imperial laser system and analysis
Emerging Active Regions: turbulent state in the photosphere
Volume 32, Issue 1, Pages (October 2001)
T18_VG2.4_Disk_#2 processing summary
A proposal for a pulsed surface heating experiment in a CLIC accelerating structure using variable pulse length Alexej Grudiev.
The Junction Diode Junction Diodes:
The Junction Diode Junction Diodes:
Presentation transcript:

T24 results and comparison to the preceding studies on CLIC prototype structures May 17, 2011 T. Higo (KEK)

X-band collab meeting at SLAC (T. Higo) Topics Processing as a whole Typical BD appearance pattern BD vs Eacc BDR evolution Comparison of BDR among structures BDR vs pulse width or pulse heating Dark current Remembrance of preceding pulses Thinking from double pulse operation Following pulses without stopping BD location 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Prototype structures at Nextef T18 TD18 TD18_quad T24 TD24 TD24R05 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Processing/operation as a whole Number of breakdowns T18 = 2500 BD / 4000 hrs TD18 = 8000 BD / 4000 hrs T24 = 1200 BD / 2000 hrs 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) T18_VG2.4_Disk #2 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) TD18 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) Processed for 1744 hours. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Typical breakdown appearance pattern Some breakdown triggers a series of following breakdowns. After a while, it becomes stable, randomly appeared. It needs usually more time to determine the BDR in a well-stable period. Sill we need better way of BDR evaluation. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) Final run at 120MV/m Not statistically stable at all for especially a low BDR period. Two categories!? Severe BD & recovery Stable regime Well statistically developed Ev31 Ev32 Time of the final point is not real. Ev30 Ev26 Ev25 Regeme not-statistically random 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Typical ACC BD and following recovery process Run35 Typical ACC BD and following recovery process Each by 1 pulse A few hundred pulses Ev26 Ev27-29 Ev30 1st pulse BD Recovery process Next ACC BD ACC BD From the beginning of a pulse Again at later in a pulse Later in a pulse 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) T24#3 Run16 goal 110MV/m at 252nsec BDR vs time 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) TD18_#2 at 252 ns TD18_Disk_#2 BDR~ 1.3 x 10-5 /pulse/m] during Run 51&52 (60MW, 252ns) as of the total RF-ON period of 2255 hours # BD 10^-6 /pulse/m BDR Still decreasing in a logarithmic time scale BDR ~ t^-0.38 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) BDR vs Eacc Exponential slope at 100 MV/m for 10MV/m T18 X10 TD18 X20 T24 X10 Power index “n” as Eaccn T18 n= 26 TD18 n=25-29 T18 n=22 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) Breakdown rate 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Relevant data points of BDR vs Eacc Steep rise as Eacc, 10 times per 10 MV/m, less steep than T18 2011/5/17 X-band collab meeting at SLAC (T. Higo)

T24 T24#3 BDR evolution at 252ns Lines are assuming the same exponential slope as that at 400hr 2011/5/17 X-band collab meeting at SLAC (T. Higo)

BDR evolution nominal at 100MV/m 252ns Exponential decrease T18 TD18 T24 400hrs 186hrs Power index “n” as (elapsed time)-x - 4.3 2011/5/17 X-band collab meeting at SLAC (T. Higo)

TD18_#2 Evolution of breakdown rate 2011/5/17 X-band collab meeting at SLAC (T. Higo)

T24#3 BDR evolution at 252ns normalized 100MV/m Assuming the same exponential slope as that at 400hr 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Comparison of BDR among structures Present status Comparison of BDR vs Eacc is just the base for feasibility evaluation. It is not easy to evaluate < 10^-7. And it is time dependent. What is the best parameter to characterize? No more than demandnig more understanding of BD (and BD trigger) mechanism. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Comparison of BDR in T18, TD18 and T24 400hrs TD18 T24 1677hrs T18 Damped 放電頻度 約100倍 温度上昇か?? T18 T24 2011/5/17 X-band collab meeting at SLAC (T. Higo)

BDR vs pulse width or pulse heating It is evident that BDT is a steep function of pulse heating. But not yet well understood when comparing various structures, and even in various stages of a structure. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

T24#3 BDR vs width in various stages 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) T24#3 BDR vs Pulse heating at 105MV/m Final at 120MV/m BDR scales as exponential to pulse heating, though BDR changes as processing and the functional form is not easy to conclude. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) TD18 based on Faya Wang BDR vs DT Undamped Damped DT BDR BDR varies exponential to DT. The amount seems very different between T18(SLAC) and T24(KEK). T24#3 at 120MV/m 温度上昇をパラメータとすると    放電頻度が統一的に見えてきた 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) Dark current 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Amount and reached level T18_Disk TD18_Disk T24_Disk Eacc for peak dark current of 10 mA 90MV/m 70MV/m 85MV/m 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Field enhancement factor as of 090515 No big change in b during RF ON = 2300 – 2900 hrs b ~ 36—38 Following the formula and parameters of the following page 2011/5/17 X-band collab meeting at SLAC (T. Higo)

TD18 Evolution of dark current till early April in TD18_Disk IPAC10 Evolution of dark current till early April in TD18_Disk 3100 hr Dark current reduced by three order of magnitude. It followed roughly modified F-N formula. The b reduced from 70 to 40 in its initial stage of processing keeping b * Esmax ~ 5~7 GV/m but became larger to 55 at the later stage. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Fitting including low current data points b=33 (252ns) b=26 (412ns) Beta seem small b = 26—33 at RF ON = 1000 hrs 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Comparison of beta values TD18 T24 Meas. at RF ON(hrs) 2300 – 2900 100 – 600  3200 1000 b 36 – 38 70  40  55 26 – 33 Seems good to compare these values. Higher beta in TD18? How it changes as time? Better to monitor systematically. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Dark current spectra T18#2 Different widths Different acc field levels 2011/5/17 X-band collab meeting at SLAC (T. Higo)

TD18 spectrum is missing. Our fault! Simply enough! It should be measured! 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) T24#3 Dark current spectra Meas. 25 Feb., 2011 @ 1400 hours after processing start 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) Dark current Dark current gives a measure on HG performance In beta In its amount Dark current contains many hints field emission site beta as a whole and possibly local beta Even though it is the result of the whole area with a limited acceptance We want to improve the monitoring As the processing proceeds, especially at the beginning 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Remembrance of the preceding pulse? Is the breakdown trigger influenced by anything from the preceding pulse or from the general situation of the period? 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Run 98 switching among three power levels for 46.2 hours TD18 Run 98 switching among three power levels for 46.2 hours 90 – 95 – 100 MV/m Switching among three power levels in each 50 pulses. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Comparison to the usual BDR data TD18 Comparison to the usual BDR data 8 1 43 Run 98 3.3*10-6 / 2.6*10-5 / 1.4*10-4 [BD/pulse/m] Data points from jumping among three levels BDR is determined by the power level of the very pulse. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) The remembrance of the preceding pulses, 50 – 100 pulses ahead, is not kept. We need to refrain the same experiment with pulse-to-pulse switching to see whether the remembrance is kept from the previous pulse. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Thinking from double pulse study What about the remembrance very close to the last pulse separated by 10 – 200 nsec period? 2011/5/17 X-band collab meeting at SLAC (T. Higo)

BDR: measured and instantaneous f(Eacc) = BDR depending on Eacc g(t) = instantaneous BDR within a pulse h(DTp) = BD potential factor determined by the integrated effect of such as pulse heating of many pulses before the BD pulse We thought that the double pulse study would give us the clue. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Features investigated by double pulse operation 5ns TE Period Width 200ns FG set value Period=210ns Width=200ns 200 + 10 + 200 FG set value Period=410ns Width=200ns 200 + 210 + 200 Double (200+10+200) = Single (410ns eq.) in TD18 Run 71 (30 June – 1 July ---) Double (200+210+200) = Single (2000 or 400ns eq.??) in TD18 Run 72, 73, 74, 89, … 2011/5/17 X-band collab meeting at SLAC (T. Higo)

TD18 Run 89 Well separated double pulse at 90 MV/m 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Run 25&26 T24#3 BDR double pulse at 110MV/m Guide line slope : BDR_former = 2.4*10^-6 BDR_latter = 3.7*10^-6 Guide line slope : BDR_former = 3.2*10^-6 BDR_latter = 4.0*10^-6 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) Run28: 200+200+200 ACC-BD ACC-BD First-pulse BD First-pulse BD 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Result of double pulse study The BDR becomes saturating after initial a few tens of hours. BDR of latter pulse is a little higher than that of former pulse, but at most within a factor 2. Former pulse BD always triggers latter pulse BD. The breakdown timing within a pulse distributes uniformly in the pulse. First-pulse BD after a BD mostly starts from the beginning of the former pulse. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Trigger for the breakdown Pulse heating at 100MV/m 200ns (DT=10degC)  400ns(DT=13-14degC) Then from width dependence BDR exponential rise as DTp (SLAC TD18) DTp=3degC h(DTp) x10 But double pulse result BDR of latter pulse = at most x2 It seems g(t) rises moderate even if rises This result supports BDR is mostly determined by non-instantaneous mechanism. i.e. no memory from the preceding pulse sepaated by 10 – 200 nsec. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Following pulses without stopping How the structure changes after “BIG” breakdown? The probability of breakdown is extremely high, but the breakdown does not always happen. The probability of the breakdown rapidly decreases as number of pulses. Structure surely remembers the BD. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Run 100 at 100 MV/m level Behavior of eight pulses after BD TD18 Run 100 at 100 MV/m level Behavior of eight pulses after BD More than 50% of breakdowns are not accompanied by any consecutive breakdowns. Some are followed by breakdowns. Correlation between number of consecutive breakdowns and the hardness of the initial breakdown should be evaluated. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) BD location 2011/5/17 X-band collab meeting at SLAC (T. Higo)

T24#3 BD location T24#3 Run 9 RF-ON=400-430 hrs 100MV/m at 252ns just after reaching Run 16 RF-ON=620-660 hrs During ramping to 110MV/m at 252ns 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) BD location Analysis program for the BD localization by RF timing has almost been developed. KEK needs careful and through analysis of BD location, back to T18 and TD18. This I was reminded by the SEM views of T18 and TD18 shown by CERN, the distribution of the arc spots and the high magnetic field spots along the structures. We have in mind but not yet done well. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) Conclusion Systematic understanding applicable to all of the structures is not established at all. We should acquire more data systematically. We should make complementally studies with simple setups depicting each a single change than reference to look at the relevant mechanism that appeared in the prototype structures. Theoretical studies are welcome in understanding and finding the strategy. 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) Additional materials 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Deduction of the field enhancement factor Fitting of modified F-N curve Assuming Es/Eacc=1.95 for T24 f(Cu)=4.52eV 2011/5/17 X-band collab meeting at SLAC (T. Higo)

X-band collab meeting at SLAC (T. Higo) Pritzkau thesis 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Study with double-pulse operation Temperature rise was calculated based on Pritzkau thesis formula. For 200nsX2 double pulse, very little difference exists in the latter pulses with different off-periods from 0 to 200ns. Big temperature difference exists only between former pulse and latter pulse T24: Former=10.1C vs Latter=13.3 ~14.3degC TD18: Former=45 vs Latter=60~63C. Let us compare the BDR between former and latter pulse!! 2011/5/17 X-band collab meeting at SLAC (T. Higo)

Double-pulse temperature rise at unloaded gradient of 100MV/m Hs=0.485MA/m at the last cell of TD18#3 Hs=0.23MA/m at the last cell of T24#2 magnetic field= 0.485 MA/m At end of full pulse 0.4 microsec temp= 63.3727 degC At end of first pulse 0.2 microsec temp= 44.8112 degC At beginniing of second pulse 0.3 microsec temp= 23.196 degC At end of second pulse 0.5 microsec temp= 60.7817 degC At beginniing of second pulse 0.4 microsec temp= 18.5614 degC At end of second pulse 0.6 microsec temp= 59.0539 degC magnetic field= 0.23 MA/m At end of full pulse 0.4 microsec temp= 14.2519 degC At end of first pulse 0.2 microsec temp= 10.0776 degC At beginniing of second pulse 0.3 microsec temp= 5.21657 degC At end of second pulse 0.5 microsec temp= 13.6693 degC At beginniing of second pulse 0.4 microsec temp= 4.1743 degC At end of second pulse 0.6 microsec temp= 13.2807 degC No significant difference in pulse heating temperatures among latter pulses, only 6%, but significant difference between former and latter, by 40%. 2011/5/17 X-band collab meeting at SLAC (T. Higo)