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IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 QuickTime™ and a decompressor are needed to see this pict 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, USA J. D. Fox, C. H. Rivetta - SLAC, USA; W. Höfle - CERN, Switzerland QuickTime™ and a decompressor are needed to see this picture. *WEOBRA02

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Page 1: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1

QuickTime™ and a decompressor

are needed to see this picture.

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

QuickTime™ and a decompressor

are needed to see this picture.

*WEOBRA02

Page 2: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

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

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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

Page 4: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

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

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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)

Page 6: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

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)

Page 7: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

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)

Page 8: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

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)

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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)

Page 10: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

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

Page 11: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

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

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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

Page 13: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

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

Page 14: IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 1 Simulation of E-Cloud driven instability and its attenuation using a

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

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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

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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.

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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

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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?

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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.

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IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 20

Backups

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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

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IPAC10, Kyoto, Japan, May 23-28, 2010 E-cloud feedback simulations - Vay et al. 22

Example: application to SPS @ 120 GeV

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SPS - W=120 GeV Electron density at station 0

Buckets 95-100 Buckets 345-350

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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

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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