beam tests of dfs & wfs at facet andrea latina, j. pfingstner, d. schulte, d. pellegrini (cern),...

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Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker, and N. Lipkowitz (SLAC) AWLC 2014 – Fermilab – May 14, 2014

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Page 1: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

Beam Tests of DFS & WFSat FACET

Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo)

With the help of F.J. Decker, and N. Lipkowitz (SLAC)

AWLC 2014 – Fermilab – May 14, 2014

Page 2: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Overview

• Motivations and objectives

• Summary of the results

• Analysis of the results

• Conclusions

Page 3: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Beam-based alignment testsWe proposed automated beam-steering methods to improve the linac performance by correcting orbit, dispersion, and wakefields simultaneously.

Our technique is:• Model independent• Global• Automatic• Robust and rapid

We base our algorithms operate in two phases: automatic system identification, and BBA

It is a considerable step forward with respect to traditional alignment techniques.

Page 4: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Recap on Dispersion-Free Steering and Wakefield-Free Steering

• DFS: measure and correct the system response to a change in energy

(we off-phased one klystron either in sectors S02 or in S04, depending on the case)

• WFS: measure and correct the system response to a change in the bunch charge

(this time we used 70% of the nominal charge, 2e10 e- and 1.3e10 e-)

Recap of the equations

Simulation: WFS weight scanSimulation: DFS weight scan

woptimal = ~40

Page 5: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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The SLAC linac

(*) Emittace measurements:• S02: 7 wires (only 5 used)• S04: quad-scan (1 wire)• S11: 4 wires (only 3 used)• S18: quad-scan (1 wire)

• Divided in 100m long sectors• Energy = from 1.19 GeV to 20.3 GeV• Bunch length = from 1.0-1.5 mm in S02 to 20 μm in S20• Nominal charge = 2e10 e- (test charge = 1.3e10 e-)• Nominal emittances: X = 2.5 x 10-5 m ; Y = 0.2 x 10-5 m

Orbit feedbacks (slow):• S03-04, S06, S11, S15: orbit correction• S09, S17-18: energy correction

* * * *

Page 6: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Overview of the tests performed

2013:1) Dispersion-Free Steering

in sectors LI04 – LI08

2014:2) Wakefield-Free Steering

in sectors LI02 – LI04

3) Wakefield-Free Steering and Dispersion-Free Steering simultaneouslyin sectors LI02 – LI04

4) WFS and DFS over longer sections of the LINACin sectors LI05 – LI11

Page 7: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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March 2013: Tests of DFSSectors LI04 thru LI08 (500 meters of Linac)• 52 correctors and 52 bpms (one every two)• Dispersion created off-phasing one klystron in sector LI03 by 90o

Dispersion got reduced by a factor 3-4 in X and Y

Page 8: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

8Before correction After 3 iterations

Incoming oscillation/dispersion is taken out and flattened; emittance in LI11 and emittance growth significantly reduced.

After 1 iteration

S19 phos, PR185 :

March 2013: DFS and Emittance Reduction

Emittance at LI11 (iteraton 1)X: 43.2 x 10-5 mY: 27.82 x 10-5 m

Emittance at LI11 (iteration 4)X: 3.71 x 10-5 m Y: 0.87 x 10-5 m

Page 9: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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March 2014: Tests of WFS in LI02-04

• We measured the wakefield effects by using a test beam with 80% of the nominal value

• We used all correctors and all bpms.

• Notice: The wakefield is measured as orbit distortion due to the difference in bunch charge

Page 10: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Tests of WFS in LI02-04, March 2014Vertical Wakefield orbit = Y_test_charge – Y_nominal

<<<

Ste

ps o

f cor

ectio

n <<

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Page 11: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Tests of WFS in Sectors LI02-04Horizontal Wakefield orbit = X_test_charge – X_nominal

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Ste

ps o

f cor

ectio

n <<

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Page 12: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Tests of WFS in Sectors LI02-04WFS convergence plot.

Apply WFS with optimal weight=40.

Emittance at start of our shift was:X = 2.79 / 1.07 x 10-5 mY = 0.54 / 1.12 x 10-5 m

Emittance after correctionX = 3.38 / 1.01Y = 0.12 / 1.16 ; 0.17 / 1.20

Nominal emittances should beX = 2.5 x 10-5 mY = 0.2 x 10-5 m

Page 13: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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WFS weight scanWeight scan vs. emittance. We tried w = 4, 40, 160, 400.

From simulation, one expects something like the black line in the plot:

Vertical emittance measured in sector 04 (quad scan)-w = 0 initial vertical emittance: 0.56 / 1.10-w = 4, vertical emittance = 0.36 / 1.63-w = 40, vertical emittance = 0.12 / 1.16 (re-measured: 0.17 / 1.20)-w = 160, emittance not measurable -w = 400, emittance not measurable

Conclusion:• Emittance scan gives expected results• No time for measuring more points

Page 14: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Sometimes in Sectors LI02-04First test of combined test of DFS+WFS. Notice machine “hiccups”.

Page 15: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Sometimes in Sectors LI02-04Test of DFS: LI02-LI04. Divergence.gain = 0.5svd = 0.7wdfs = 40

Page 16: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Tests of simultaneous DFS + WFS in LI05-LI11Problems:• Very unstable machine

• Damping ring extraction kicker• NRTL energy jitter• Earthquake ?

• Initial config problems with scavenger line (3h to recover)

Emittance at shift start:- X = 4.186 / 1.1- Y = 0.445 / 1.06

Emittance 6h later, before applying BBA- X = 11.21 / 1.19- Y = 0.91 / 1.12

Emittance after correction:- X = 9.50/1.04- Y = 1.06/2.40 (improvement in X)

Not conclusive

Page 17: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Tried a few interesting things:1) simultaneous X and Y correction2) with all coupled information3) re-measurement of the golden orbit after 5 or 6 iterations, to update the

reference for the orbit correction, y0

Emittance Y:--> from 1.58 x 10-5 m vertical emittance before correction4) down to 0.50 after few iterations of fully coupled correction5) to further 0.40 after resetting the target orbit during the correction

(equivalent to correcting without orbit constraint)

Further tests in Sectors LI05-11Extra beam-time

Page 18: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Analysis

• Try to understand divergence in simulation (see next slides)

• Stability analysis proved that the choice of gain, g was correct, and that the system is stable even in presence of potential corrector errors:– bn : bpm readings at iteration n

– δn: relative correction– R: ideal response matrix– R tilde: erroneous matrix representing eventual corrector erroes

if the absolute value of all eigenvalues of (I-gRR) < 1, the system is stable

Page 19: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Singular Values, DFS+WFS, w=40

Page 20: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Correcting a simulated LINACwith the measured response matrices

…including:

• Injection jitter• Misalignments• BPM resolution error (3 microm)• Transverse and Longitudinal Wakefields

Picking N progressive singular values at time

Page 21: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Correction using N=2 singular values

norm_OrbitX = 8.13995norm_OrbitY = 25.8351norm_DispX = 1.29383norm_DispY = 2.99051norm_WakeX = 0.905165norm_WakeY = 1.17392

Page 22: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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N=3 singular valuesnorm_OrbitX = 10.3687norm_OrbitY = 22.6852norm_DispX = 1.53973norm_DispY = 3.02105norm_WakeX = 0.729164norm_WakeY = 0.998268

Page 23: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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N=4 singular valuesnorm_OrbitX = 7.61432norm_OrbitY = 19.1609norm_DispX = 1.03749norm_DispY = 1.40887norm_WakeX = 0.50546norm_WakeY = 0.734156

Page 24: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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N=5 singular valuesnorm_OrbitX = 6.72384norm_OrbitY = 22.656norm_DispX = 0.811785norm_DispY = 1.34545norm_WakeX = 0.380037norm_WakeY = 0.869225

Page 25: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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N=6 singular valuesnorm_OrbitX = 7.31326norm_OrbitY = 23.0469norm_DispX = 1.04246norm_DispY = 1.38634norm_WakeX = 0.435169norm_WakeY = 0.917698

Page 26: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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N=7 singular values

Page 27: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Singular Values, DFS+WFS, w=40

Page 28: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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FACET-specific problems

• The response matrix measurement is very slow– Takes ~2 hours for 48 correctors / 1 matrix

• Large jitter in the horizontal axis makes the X axis harder– Damping ring extraction kicker– RF system of NRTL bunch compressor

• Machine “hiccups“, LEM– LEM (linac energy management) http

://www.slac.stanford.edu/grp/ad/op/LEM/index.shtml– Impact to be studied

Page 29: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Speeding up the response matrix measurement

1) While measrung the response of dispersion in S02-S042) Optimize speed in measurements3) Test a feed-forward system to stabilize the orbit during correction

Worked with Nate Lipkowitz to speed up the system identification procedure.

Overall 30% speed up measured

Time required to set corrector and read bpms

SPEED UP ACCOMPLISHED.

Still quite slow.

Page 30: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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New tools developed“CERNBBA” Tools:

(top) System Identification(bottom) Beam-Based Alignment

Tests foreseen at Fermi (Elettra) and ATF2 (KEK), …

Page 31: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Conclusions and future plans• Applying DFS and WFS, the vertical emittance got reduced almost

systematically• Horizontal axis more difficult

• Sometimes observed instability/divergence:• Might be related to noise in the measurement of the response

matrices (counteracted with SVD cuts)• Tests of convergence showed that the matrices are not ill-

conditioned

• We are pursuing tests at other facilities (Fermi in Trieste, ATF2)• We will learn a lot from these tests

• Further tests at FACET should surely be envisaged• Need to speed up the system identification phase

Page 32: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Extra

Page 33: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Shift 4 – Sunday – Sectors LI05-11

Test of DFS+WFS followed by WFS only• Iteration 1-7 (including): DFS+WFS

• corresponding to previous plot blow)• Iteration 8-10 (including): drift (gain=0)

• corresponding to previous plot blow)• Iteration:11-18 (including): WFS (setting DFS gain to 0)• Iteration 13: some kind of machine hickup (not identified). Algorithm recovers afterwards• Emittance non measureable in Y – we stopped

Page 34: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Response 0: nominal orbit

X Y

Page 35: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Dispersion response: R1-R0

Wakefield response: R2-R0X Y

X Y

Page 36: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Singular values for X and Y

2 very large singular values – we need to understand what they do represent

Page 37: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Response 0: rms jitter vs max excitation

Page 38: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

38Removed vertical BPM 46

Response 1: rms jitter vs max excitation

Page 39: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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Response 2: rms jitter vs max excitation

Page 40: Beam Tests of DFS & WFS at FACET Andrea Latina, J. Pfingstner, D. Schulte, D. Pellegrini (CERN), E. Adli (Univ. of Oslo) With the help of F.J. Decker,

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