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IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1
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Simulation of E-Cloud driven instability and its attenuation using a feedback system in the CERN SPS*
J.-L. Vay, J. M. Byrd, M. A. Furman, R. Secondo, M. Venturini - LBNL, USAJ. D. Fox, C. H. Rivetta - SLAC, USA; W. Höfle - CERN, Switzerland
Simulation of E-Cloud driven instability and its attenuation using a feedback system in the CERN SPS*
J.-L. Vay, J. M. Byrd, M. A. Furman, R. Secondo, M. Venturini - LBNL, USAJ. D. Fox, C. H. Rivetta - SLAC, USA; W. Höfle - CERN, Switzerland
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*WEOBRA02
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 2
The problem
Transverse instability observed in SPS beams due to electron clouds
Interaction between e-cloud and beam leads to large transverse oscillations
Feedback system was proposed to control the beam transverse motion
We use the Particle-In-Cell framework Warp-Posinst to investigate dynamics of instability as well as feasibility and requirements of feedback
Pipe
e-
gas
e-
bunch 1
bunch 2
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 3
Our simulation framework encompasses the Warp and Posinst PIC codes
2-D slab of electrons
3-D beam sproc 1 2 N/2 N/2+1 N-1 NStation n n+1 n+N/2-1 n-N/2 n+N-2 n+N-1
Warp quasistatic model similar to HEADTAIL, PEHTS, QuickPIC.
parallellized using pipelining
Mesh refinement provides higher efficiency Secondary emission from
Posinst:
- enables self-consistent multi-bunch calculations.
Example: - 2 bunches separated by 25 ns in SPS
36 35 Beam ions
Electrons Beam directionBeam direction
side view
top view
side view
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 4
Physics of electron interaction with bunches
Beam directionBeam direction
1. Electrons injected here from Posinst dump
1. Electrons injected here from Posinst dump
Beam density (x1015) at t=0 (bunches 35-36 = buckets 176-181)
chamber wall
3D view
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 5
Physics of electron interaction with bunches
2. Electrons are focused by bunch
2. Electrons are focused by bunch
chamber wall
3D view
Electron density (x1012m-3) at turn 500 (bunches 35-36 = buckets 176-181)
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 6
Physics of electron interaction with bunches
3. High-density spikes eject electron jets
3. High-density spikes eject electron jets
chamber wall
3D view
Electron density (x1012m-3) at turn 500 (bunches 35-36 = buckets 176-181)
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 7
Physics of electron interaction with bunches
4. Secondary emission from impact of e- jets on walls
4. Secondary emission from impact of e- jets on walls
chamber wall
3D view
Electron density (x1012m-3) at turn 500 (bunches 35-36 = buckets 176-181)
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 8
Physics of electron interaction with bunches
5. Electrons fill the chamber5. Electrons fill the chamber
chamber wall
3D view
Electron density (x1012m-3) at turn 500 (bunches 35-36 = buckets 176-181)
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 9
Physics of electron interaction with bunches
6. Electrons interact with next bunch
6. Electrons interact with next bunch
chamber wall
3D view
Electron density (x1012m-3) at turn 500 (bunches 35-36 = buckets 176-181)
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 10
Electrons after 500 turns
chamber wall
Electron density (x1012m-3) at turn 500 (bunches 35-36 = buckets 176-181)
3D view
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 11
Bunches 35 and 36 after 500 turns
chamber wall
Beam density (x1015m-3) at turn 500 (bunches 35-36 = buckets 176-181)
3D view
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 12
Fra
ctio
nal t
une
Comparison with experimental measurements
Separation in two parts, core and tail, with tune shift in tail higher than in core Similar tune shift for the core of the beam but higher with simulations for tail More experimental results at poster WEPEB052, J. D. Fox et al, “SPS Ecloud
instabilities - Analysis of machine studies and implications for ecloud feedback”, Wednesday, May 26, 16:00-18-00.
Experiment Warp-PosinstBunch 36, Turn 0-100Bunch 119, Turn 100-200
head tail head tail
Fra
ctio
nal t
une
Z slice
Nominal fractional
tune=0.185
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 13
Comparison with experimental measurements - 2
Both expt. and sim. show activity level inversely proportional to frequency
Interesting difference: instability grows in simulation but is already there at turn 0 in experiment
Experiment Warp-Posinst
Turn
Turn
Fre
q. [
GH
z]F
req.
[G
Hz]
Spectrum bunch 35
Spectrum bunch 36
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 14
Bunches transverse internal structure has fairly long wavelength component
• Can a feedback system resolving the bunch control the instability?
• What characteristics are needed, (amplitude, frequency range, noise level, delay, …)?
m-3
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 15
Simulated feedback model
• Ef is set from estimated velocity offset vy:
• predicts y’(t)=vy /vz from records of centroid offsets at two previous turns yi-1(t) and yi(t) using linear maps, ignoring longitudinal motion and effects from electrons
Ef
Lf
vz
zy
vy = (q/m) Ef Lf /vz
Kick in transverse velocity
Ef = gvy (m/q) vz / Lf g
i -1i
i +
with
In following results, =1.(for =0, same as Byrd PAC95 and Thompson et PAC09)
SPS
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 16
Emittance history with feedback on/off, with gains g=0.1 and 0.2
Feedback very effective at damping instability.
Better with g=0.2 for bunch 36.
Run with bunch 35 frozen.
Effect of bunch 35 on 36 is weak.
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 17
Tests with finite bandwidth
Runs with 5 different digital filters with cutoffs (-3 dB) around 250,
300, 350, 450 and 575 MHZ.
With these filters, cutoff>450 MHz needed for maximum damping.
cutoff
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 18
Multi-bunch simulations: beware of electron injection procedure.
Run of bunch (36,37) gives same emittance histories as (35,36).
Single bunch runs with electron load (a) Uniform(b) Random refreshed at each time step(c) Random using load from t=0
=> Bunch 36 experienced more noise than 35 because of random secondary electron generation.
Why is emittance of 36 >> 35?
Is it because <ne> raises by ~8%? Source of inconsistency?
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 19
Summary and future work
Beam-ecloud self-consistent simulations are now within reach, allowing detailed understanding of the dynamics and control of beam instability via feedback systems.
Improvements to Warp-Posinst quasistatic model
• mesh refinement,
• secondary emission, gas ionization,
• better feedback model.
Multi-bunch simulations are now possible (thanks in part to parallelism).
Good qualitative and semi-quantitative agreement with experiment.
Modeling of bunches 35 and 36 in SPS at 26 GeV show effective damping from simulated feedback, provided that bandwidth cutoff>450 MHz.
Care must be exercised with interpretation due to statistical implications of electrons injection procedures.
A lot more work is needed, including: implementation of planed feedback n-tag prediction, filtering, etc; better control of numerical noise issue in simulations, eventually using as proxy to emulate real machine noise; replace smooth focusing with linear optics, etc.
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 20
Backups
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 21
Physics of electron interaction with bunches
Beam directionBeam direction
1. Electrons injected here from Posinst dump
1. Electrons injected here from Posinst dump
Electron density (x1012) at t=0 (bunches 35-36 = buckets 176-181)
2. Electrons are focused by bunch
2. Electrons are focused by bunch
3. High-density spikes eject electron jets
3. High-density spikes eject electron jets
4. Secondary emission from impact of e- jets on walls
4. Secondary emission from impact of e- jets on walls
5. Electrons fill chamber and interact with next bunch
5. Electrons fill chamber and interact with next bunch
chamber wall
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 22
Example: application to SPS @ 120 GeV
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 23
SPS - W=120 GeV Electron density at station 0
Buckets 95-100 Buckets 345-350
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 24
Larger 3D view of electron density at t=0(buckets 95-100)
Beam directionBeam direction
Electrons injected here from Posinst dump
Electrons injected here from Posinst dump
IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 25
Added model for kicker
E
L
vz vy = (q/m) E L/vz
Kick in transverse velocity
Kick is at fixed station and is on/off on turn basis.
From betatron tune , can infer induced maximum displacement y= vy/vz
Example: SPS at injections (26 GeV) L = 37.5 cm = 71.87 For a field of 10 kV/m, the beam
maximum displacement is ~10 m.
zy