4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)
description
Transcript of 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)
![Page 1: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/1.jpg)
Discussion on critical issues for testing:
breakdown identification, preparation for test, processing protocol, etc.
4th Annual X-band Structure Collaboration MeetingMay 3, 2010T. Higo (KEK)
![Page 2: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/2.jpg)
The purpose and way of this timeslot
• I want the present discussion to focus on the high gradient performance evaluation of main linac accelerator structures for CLIC.
• I picked up some view graphs so that you are triggered to present comments and discussions.
• To do items 1—10 appeared here are those we think needed for KEK activities, but also common to all this community.
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 2
![Page 3: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/3.jpg)
To do1. Summarize the present processing early stage2. Get BDR from medium field level3. Take BRD values carefully in statistical manner in mind4. Evaluate the evolution of BDR5. Try to correlate BDR with other observed results6. Measure dark current to monitor processing7. Evaluate for whole life of accelerator structure8. Do more with post-mortem by SEM9. Do tests with simple geometries10. Work hard to conclude present-day feasibility description
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 3
![Page 4: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/4.jpg)
For completing feasibility study• Requirement for CLIC• Requirement for linear collider• Requirement for other applications
• Following discussions are for LC especially CLIC• Items needed for feasibility judgment
• Is it enough with evaluation items of on-going high gradient tests?
• Let us consider what we need and what we can.
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 4
![Page 5: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/5.jpg)
What are needed to evaluate for judging the feasibility
• Fabrication and preparation until feeding power– Required processes, associated time and cost, …..
• Performance in processing without beam– Processing speed– Ultimate reach of Eacc field– Breakdown rate vs Eacc
– Evolution of breakdown rate– Breakdown rate vs pulse width/shape– Dark current– Damage during processing
• Performance with beam• Deterioration due to long-term operation
2010/5/3 54th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 6: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/6.jpg)
We have started a series of tests on 11.4GHz prototype structures
T18_#1 T18_#2 T18_#3 T18_#4 TD18_#1 TD18_#2
Cell make KEK KEK KEK KEK KEK KEK
Bonding SLAC SLAC SLAC SLAC SLAC SLAC
Test SLAC, done
KEK, done
SLAC, done
KEK, future
SLAC, in test
KEK, in test
2010/5/3 64th annual X-band structuture collaboration meeting at CERN (T. Higo)
We have also tested two quadrant type structures.
Let us take these examples in mind and optimize our tests in near future including 12GHz structures.
![Page 7: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/7.jpg)
Basic studies with simple setup are ongoing
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 7
Single-cell C10/CD10 Waveguide DC spark Pulse heating
SLAC SLAC SLAC / KEK CERN SLAC
SW TW TW DC SW
On-going On-going Sleeping On-going On-going
These also are already on-going and let us extend these to complement the tests with prototype structures and help understand physics behind the results.
![Page 8: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/8.jpg)
BackgroundAccelerator design in mind
• How high can / should the gradient be?– CLIC sets 100MV/m for 3TeV– We should ask ourselves whether it can be realized and when? – For a certain timing of the project, we should declare the
practical value. – Should it be 100? Can it be lower or higher?
• Tolerable breakdown rate?– During processing? – Through the accelerator life?
• What HOM performance is required?– Big interrelation between pulse heating and damping geometry
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 8
![Page 9: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/9.jpg)
Key technical issues should be understoodin fabrication and preparation until feeding power
• Do we need diamond turning?• Do we need high temperature vacuum treatment of
material?• Do we need hydrogen high temperature process?• Do we need vacuum baking at 650C for a week?
• All these should be confirmed with dedicated tests to understood in their mechanisms to confirm.
• This can be accomplished by the systematic basic tests in addition to a series of prototype structure tests.
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 9
![Page 10: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/10.jpg)
What can/should we learn from processing without beam?
• Higher field toward downstream– Especially in T18/TD18
• What is RF processing? Why do we need it?– Improvement or deterioration?– Inevitable process? – Can it be replaced by careful preparation?
• Breakdowns are inevitable? Tolerable amount?– Tolerable number of breakdowns– Tolerable breakdown size
• What determines the processing speed?– Ramping speed for recovery from fault
• Waiting time• Recovery path (width, power, others ….)
2010/5/3 104th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 11: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/11.jpg)
Difference in processing speed exists
• Processing speed– One of the important characteristics– Compare it w.r.t. time or #BD?– We should compare among experiments
• Breakdown identification is related– Related to how to identify breakdowns
• Missing energy (SLAC), current flush (KEK)• RF reflection, RF transmission• Need to critically compare, but not yet done fully
• Processing protocol is also related– Speed and path of recovery from BD
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 11
![Page 12: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/12.jpg)
TD18_#2 test at KEKSome pulse: Run34 #38 and #39
This case was not analyzed reasonably.
F Rs Ra Tr
FC-UP FC-Mid I_Rs Q_Rs
2010/5/3 124th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 13: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/13.jpg)
0 50 100 150 200 250 3000
20
40
60
80
100
120
BKD Rate (hr-1)Average gradient (MV/m)
50 ns 100 ns 150 ns 200 ns
This time, processed structure by progressively lengthening the pulse at constant gradient (110 MV/m)
Second T18 Structure Tested at SLACT18_#3 Chris Adolphsen, CLIC09
2010/5/3 134th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 14: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/14.jpg)
Whole history of processing of T18_VG2.4_Disk #2
0
20
40
60
80
100
120
0
500
1000
1500
2000
2500
3000
0 500 1000 1500 2000 2500 3000 3500 4000
MasterTable_Eacc_Trend till_090610
<Eacc> 51nsec Ushi<Eacc> 113ns Ushi<Eacc> 173n ushi<Eacc> 213n Ushi<Eacc> 253ns UshimotoEacc keep 253ns UshiEacc 51ns UshiEacc 113ns UshiEacc 173ns UshiEacc 213ns UshiEacc 253ns UshiEacc Usahimoto 2/21-3/23Eacc 252ns Usahi 4/1-4/7Eacc 252ns 4/7-14Eacc 312ns 4/14-16Eacc 412ns 4/23-27Eacc 331ns 4/28-5/1Eacc 252ns 5/1-11Eacc 412ns 5/11-6/10
Total BD<Eacc> MV/m Total# BD
RF-ON integrated (hr)
090610T18_#2, T. Higo
2010/5/3 144th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 15: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/15.jpg)
High Power Test begin at 12/03/2009 15:00
0 100 200 300 400 500 600 700 800 900 10000
20
40
60
80
100
120
Accumulated rf process time (hr)
BDR (1/hr)<G> for regular cell (MV/m)Pulse Width (divided by 10 ns)
TD18_#3 Faya Wang, 10 March 2010
2010/5/3 154th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 16: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/16.jpg)
Tp50ns250ns
TD18_#2, S. Matsumoto, in this meeting
2010/5/3 164th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 17: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/17.jpg)
To do -1
• These are some of recent examples.
• Let us summarize such processing characteristics
• And try to identify the driving source of difference– The way of processing or the structure itself?
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 17
![Page 18: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/18.jpg)
We have done a series of tests on prototype structures
2010/5/3 184th annual X-band structuture collaboration meeting at CERN (T. Higo)
T18_#1 T18_#2 T18_#3 T18_#4 TD18_#1 TD18_#2 TD18_#3 Quad_#? Quad_#5Type Disk Disk Disk Disk Disk Disk Disk Quad QuadMake KEK/SLAC KEK/SLAC KEK/SLAC KEK/SLAC CERN KEK/SLAC KEK/SLAC CERN KEK
Material OFC OFC OFC OFC OFC OFC OFC OFC CuZrTest SLAC KEK SLAC KEK SLAC KEK SLAC SLAC KEK
Status Done Doen to be tested Done under test Done Done Done
#BD till goal 2000 280 * 1500 80 Hrs till goal 4000 3300 # 6000 800? Trip source ME FC ME ME FC ME ME FC
Total number of BD 4000 >2000 $
*Till reaching 200ns#Before next width, stay before BDR<1/hr$On-going
MEMissing energyFCFaraday cup current burst
Goal100MV/m with >230ns
Should compare these processing-related values in a systematical manner.
![Page 19: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/19.jpg)
Let us think What drives the processing?
• Number of breakdowns?– Surface processing through breakdowns
• RF processing time?– Field emission makes surface modification?
• Higher gradient or longer pulse operation?– Through higher dark current?
• Introduction of other perturbation?– Hot spot?
2010/5/3 194th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 20: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/20.jpg)
Is the present processing protocol the best?
• Any difference in its final performance– depending on the different protocol?
• Difference in such as – Peak power ramping speed during recovery– Width reduction and re-widening (SLAC)?
• Can we propose a processing in actual LC?– Any difference from what we do now?
2010/5/3 204th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 21: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/21.jpg)
How to define the ultimate field reach and operation level
• A significant deterioration may starts above some level in pulse energy or in peak power– Very stable operation may be possible before suffering from
many breakdowns– For example, see an experiment in DC spark test in next page
• Where should we stop further processing?– In case we can live within the level.
• Should we evaluate the performance step by step from lower field level?– See a simple schematic in peak power ramping and BDR
evaluation
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 21
![Page 22: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/22.jpg)
Etched vs. Mirror surface
and BD field seems to be stable at the beginning.The first BD field is very high (~ 450 MV/m)
It seems to take longer time until saturation.The first BD field is low.
K. Yokoyama, private communication
2010/5/3 224th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 23: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/23.jpg)
Should confirm lower level operation
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 23
Evaluate lower level operation without (before) severe damage in peak power or in pulse energy ?? to confirm the robust and well-established levelThen go higher to evaluate at the nominal value with trying to detect when the deterioration starts
609080
100 110 Target120
![Page 24: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/24.jpg)
To do -2
• Taking these consideration,
• Let us evaluate the BDR evaluation before reaching to the goal of 100MV/m
• Try to find the point over which deterioration starts (and possible the reason/mechanism)
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 24
![Page 25: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/25.jpg)
Breakdown rate evaluation
• BD identification is needed• It changes in time• BD behaves in a statistical manner• …..
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 25
![Page 26: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/26.jpg)
BD identification and threshold setting
MEReflectionFC current
2010/5/3 264th annual X-band structuture collaboration meeting at CERN (T. Higo)
In missing energy (SLAC) or current flush (KEK), or ??
OR
We should confirm the distribution and the threshold position. Do we have clear experimental evidence? Do we have information below threshold? Do we have any deterioration below threshold?
![Page 27: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/27.jpg)
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 27
TD18_Disk_#2
Almost all confirmed to be spurious
![Page 28: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/28.jpg)
To do -3
• Let us evaluate the present situation of how we identify breakdowns in a quantitative manner
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 28
![Page 29: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/29.jpg)
Deduction of breakdown rate• = #BD/period?• We should be careful when to read the BDR values.
– Breakdowns appear in an irregular manner in time.– Some breakdown triggers following breakdowns in very
short time intervals.– Are the BDR values well saturated in a statistical view point?– In a smaller value case, the error is large due to limited time
to count many BD’s.• Evaluation period long enough?
– Even not, we should extract data. Just be careful to read and use these data points.
2010/5/3 294th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 30: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/30.jpg)
Breakdown rate measurements at 252ns
0.00 5.00 10.00 15.00 20.00 25.00 30.00 0.000
10.000 20.000 30.000 40.000 50.000 60.000 70.000 80.000 90.000
100.000
Run 34 (60MW)80 BD’s BDR [10^-6 /pulse/m]
0.00 10.00 20.00 30.00 40.00 50.00 60.00 70.00 0.000
5.000
10.000
15.000
20.000
25.000
30.000
Run 35+36 (55MW)41 BD’s BDR [10^-6 /pulse/m]
TD18_#2, S. Matsumoto, in this meeting
2010/5/3 304th annual X-band structuture collaboration meeting at CERN (T. Higo)
Run 45 (60MW) 59 BD's BDR [10^-6 /pulse/m]
0.00 5.00 10.00 15.00 20.00 25.00 30.00 35.00 40.00 0.0
50.0
100.0
150.0
200.0
250.0
300.0
Run 46 (55MW) 10 BD's BDR [10^-6 /pulse/m]
0.00 10.00 20.00 30.00 40.00 50.00 0.0
5.0
10.0
15.0
20.0
25.0
1st meas. 2nd meas.
![Page 31: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/31.jpg)
Cascaded BDR Test at 100 MV/m @ 200ns
1 2 3 4 5 6 70
0.1
0.2
0.3
0.4
0.5
0.6
0.7
Frac
tion
of b
reak
dow
n ev
ents
Cascaded events
All eventsMulti-event taken as one event
Type 1 2 3 4 5 6 7
Events 77 23 5 5 1 2 1
33 hrs for the total test.
180 185 190 195 200 205 210 215
2468
pulses
Inpu
t ref
(arb
.u.)
24 26 28 30 32 34 362468
1012
pulses
Inpu
t ref
(arb
.u.)
150 160 170 180 190 200 2100
5
10
15
pulses
Inpu
t ref
(arb
.u.)
155 160 165 170 1752468
1012
pulses
Inpu
t ref
(arb
.u.)
TD18_#3 Faya Wang, 17 March 2010
2010/5/3 314th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 32: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/32.jpg)
Actual evolution of breakdown frequency
• Should evaluate the evolution in time– Keep decreasing?– Gets saturated? When? Why?– Any unexpected increase happens?
• Total number of breakdowns in life – should be expected from above information
• Speedup the evaluation– Evaluation at higher level may suffer from onset of severe
deterioration?– But we do not have any practical way to get precise data.
What to do?
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 32
![Page 33: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/33.jpg)
95 100 105 110 11510
-7
10-6
10-5
10-4
Unloaded Gradient: MV/m
BK
D R
ate:
1/p
ulse
/mBKD Rate for 230ns
250hrs
500hrs
1200hrs
900hrs
500 1000 150095
100
105
110
115
Time with RF on: hrs
Gra
dien
t: M
V/m
Gradient at 2e-6/pulse/m for 230ns pulse
Experiment DataPower Fit
Gradient Increase Over Time at a Constant Breakdown Rate
Hot Cell Flare-up
First T18 StructureTested at SLAC
T18_#1 Chris Adolphsen, CLIC09
2010/5/3 334th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 34: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/34.jpg)
BDR evolution with rf process
0 500 100010
-7
10-6
10-5
10-4
10-3
Accumulated rf process time (hr)
BD
R (1
/pul
se/m
)
100MV/m@100ns100MV/m@150ns100MV/m@200ns100MV/m@230ns
0 1000 2000 300010
-7
10-6
10-5
10-4
10-3
Accumulated rf breakdown
TD18_#3 Faya Wang, 10 March 2010
2010/5/3 344th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 35: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/35.jpg)
Breakdown rate
10-7
10-6
10-5
10-4
80 85 90 95 100 105 110 115 120
T18_VG2.4_Disk #2Breakdown rate for 252ns and 412ns
BDR(ACC) 412ns
BDR(ACC) 252ns
BDR(ACC) [1/pulse/m]
Eacc [MV/m]
0530-0610 (3700hr)
0525-0530 (3500hr)
0520-0525 (3500hr)
0515-0518(3400hr)
0511-0515 (3300hr)
0501-0507(3100hr)
0423-0427(2900hr)
0411-0414 (2800hr)
0403-0407 (2700hr)
0402-0403 (2700hr)
0401-0402 (2700hr)
0313-0323 (2500hr)
0227-0305(2300hr)
(700-1200hrs)
T18_#2, T. Higo,
2010/5/3 354th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 36: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/36.jpg)
To do -4
• Let us evaluate the evolution of breakdown rate
• Try to see whether it keeps decreasing or gets saturated or it deteriorate from some point?
• It needs long period operation, rather than tasting too many structures quickly. (I admit though that the latter is effective in some purpose.)
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 36
![Page 37: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/37.jpg)
Breakdown rate vs pulse width/shape
• Evaluation as function of– Pulse heating temperature rise– Any other thought?
• These trials are important– for understanding the mechanism of trigger of BD
• Results are consistent or understandable?– With other observations?
• Breakdown location?• Breakdown timing in pulse
– Period of irradiation with RF before BD
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 37
![Page 38: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/38.jpg)
BDR Pulse Heating Dependence
20 30 40 50 60 70 80 90 10010
-7
10-6
10-5
10-4
10-3
Peak Pulse Heating at Last Cell (K)
BD
R (1
/pul
se/m
)
T18, 900 hrsTD18, 100 MV/m @ 100ns,870hrsTD18, 100MV/m@ 150ns, 960hrs TD18, 100MV/m@200ns, 750hrsTD18, 115MV/m@150ns, 550hrsTD18, 120MV/m@150ns, 570hrsTD18, 100MV/m@230ns, 700hrsTD18, 105MV/m@230ns, 680hrsTD18, 100MV/m@50ns
TD18_#3 Faya Wang, 17 March 2010
2010/5/3 384th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 39: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/39.jpg)
Breakdown distribution at different stage
0 5 10 15 200
50
100
150
200
250
Regular Cell No.
BD
R E
vent
s
0 ~ 200 hrs200 ~ 400 hrs400 ~ 600 hrs600 ~ 700 hrs700 ~ 960 hrs 0 ~960 hrs
TD18_#3 Faya Wang, 10 March 2010
2010/5/3 394th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 40: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/40.jpg)
Timing statistics for Rs rise and Tr fall
Rs: 100—350ns for 252nsec pulse Most of Rs change sit around 360+-50nsec
Tr: 150—400ns for 252nsec pulse Most frequent when approaching to the end, from 300 to 370ns. There is a small bump at 170 nsec, at the beginning of pulse.
2010/5/3 404th annual X-band structuture collaboration meeting at CERN (T. Higo)
TD18_#2, T. Higo,
This Tr reflects the information of irradiation period before BD
![Page 41: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/41.jpg)
2010/5/3 414th annual X-band structuture collaboration meeting at CERN (T. Higo)
TD18_#2, T. Higo,
Should revise the resolution of the analysis of BD location
BD location.
![Page 42: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/42.jpg)
To do -5
• Try to correlate the BDR to other observables– Such as pulse heating – Pulse width and pulse shape– Breakdown location– Breakdown timing
• To understand the trigger mechanism to drive breakdowns
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 42
![Page 43: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/43.jpg)
Pulse-to-pulse stable dark current
• Important to measure the evolution?– Amount of FE current– Beta values in FN – Decrease and saturation, or jump up?– Can be one of the measures of processing?
• Energy spectrum– To understand the FE position information– Possible relation to trigger of BD
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 43
![Page 44: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/44.jpg)
TD18_#2Dark current evolution
especially at early stage of processing
2010/5/3 444th annual X-band structuture collaboration meeting at CERN (T. Higo)
TD18_#2, S. Matsumoto, in this meeting
![Page 45: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/45.jpg)
To do -6
• Dark current should be observed as processing proceeds
• Try to find relation between stable FE current and reached high gradient performance
• To get relation between dark current to processing.
• This information may give us a way to monitor processing.
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 45
![Page 46: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/46.jpg)
Damage during processing or in operation• Deterioration are observed
– Cell frequency change• Especially non-uniform change: not easy to compensate
– Breakdown pits and rough surface profile• Larger field enhancement?• Cleaner surface?• Hard surface due to rapid cooling?
– Triggers to the following breakdowns• Degree of deterioration should be evaluated
– Easily subject to the systematic error in measurement– Well-established setup should be used
2010/5/3 464th annual X-band structuture collaboration meeting at CERN (T. Higo)
![Page 47: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/47.jpg)
T18_Disk_#2 Bead pull amplitude plot before and after high power test
472010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo)
1. Some Eacc smoothness was deteriorated.2. Average frequency increased by 1.1MHz after 4000 hours
processing with 2500 breakdowns in total. 3. 1MHz ~40degrees/structureShould carefully measure to evaluate the effect.
![Page 48: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/48.jpg)
Performance with beam• Field profile along structure changes
– Especially on T18 or TD18– Long-term stability is to be determined with beam
• Evaluation is needed with/without beam– On BDR– On BD location
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 48
![Page 49: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/49.jpg)
Long-term operation• We should confirm the life-time stability
– The stability against practically long-enough operation at nominal field
• How to do it?– Design a structure with the same Es and Hs distribution without
beam as those with beam and test it without beam– Let us operate for full 2 months (1500hrs)
• At 10% higher field to gain x10 BDR• To simulate 2 years operation to estimate 10 year run• We can also get evolution information if exists
– Finally should inspect RF characteristics and proceed SEM inspection
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 49
![Page 50: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/50.jpg)
To do -7
• Evaluate possible damage on structure due to processing
• Design a structure with nominal loaded Ea distribution without beam
• Estimate the stability over lifetime range
• To estimate the life time history of accelerator structure.
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 50
![Page 51: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/51.jpg)
SEM inspection after high gradient test
• Postmortem inspection– Optical seems not enough, though non-destructive– SEM seems most powerful, though destructive for other than quad
• What should we evaluate– Any foreign objects? Try to find possible source!– Surface deterioration?
• On high electric field area• On high magnetic field area
• We should cut and see with SEM on the structures– T18_Disk_#1, #2, TD18_Disk_#2, #3?– Unless we have clear idea for another experimental plan
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 51
![Page 52: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/52.jpg)
To do -8
• Let us proceed post-mortem inspection by SEM on most of the tested structures unless we have clear idea what to be tested in future
• Try to correlate this inspection to the obtained high gradient performance
• To convert a dead body into birth of another life!
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 52
![Page 53: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/53.jpg)
Simple-geometry studies are needed for understanding the results on prototype structures
• Single-cell SW breakdown study– Performance taken from moderate field level (~80?)
• Milled cell• LG cell• Quad• Heavy damping• Etc.
• Modified C10/CD10 in 10 cell setup– SW needed?– TW
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 53
![Page 54: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/54.jpg)
Evaluation of effect of damping port
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 54
vs orMed. Heavy
damp Heavy dampDDS
U U D U D U D U D
U U D U D U D U D
C10-modified
SW or TW in C10-modified
![Page 55: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/55.jpg)
To do -9• Let us plan a series of high gradient test with
simple geometries from moderate field level• Try to correlate the results to the performance
observed in full-size prototype structures
• This should serve us with not only the understanding of the intrinsic limit but also some hints to go another direction to further higher gradient.
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 55
![Page 56: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/56.jpg)
In summary: My conclusion with deferring to discussion
• Essential evaluation measure is still– BDR and early processing characteristics
• More information is needed to judge feasibility– Dependence on pulse shape– Evolution and estimated change in lifetime scale– Effect of beam loading– Long-term stability
• Simple-geometry studies must to be done– In parallel to understand the mechanism and physics– Single-cell or several to 10 cell setup– SW and TW
• Study at the moderate field level should be done– before addressing higher and target operation level
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 56
![Page 57: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/57.jpg)
X-band strategy to take now• We need to show the feasible level based on now.• Characterize the structures of present-day design
(TD24) in low-60?, medium-80, goal-100, and higher-110 gradient levels.
• Conclude by ourselves the present-day feasibility of accelerator structures based on copper material.
• Show to outside world the feasibility at each field level.– Established level + level to be confirmed in near future, …..
• Then after, explore further developments including other design and other material or surface treatments.
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 57
![Page 58: 4 th Annual X-band Structure Collaboration Meeting May 3, 2010 T. Higo (KEK)](https://reader031.fdocuments.in/reader031/viewer/2022012919/568161a5550346895dd16229/html5/thumbnails/58.jpg)
Last to do -10
• Work hard with enjoying finding physics– Not only in a systematically well-organized manner for
CLIC– But also with various different view points to understand
the physics behind
• This is to conclude the feasibility– Of present-day established level– And judgment on 100MV/m– And possible idea to higher gradient
2010/5/3 4th annual X-band structuture collaboration meeting at CERN (T. Higo) 58