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Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 1/27
Instabilities Simulations with Wideband Feedback Systems: CMAD, HeadTail,
WARP
K. Li 1, H. Bartosik 1, J. Cesaratto 2, J. D. Fox 2, W. Höfle 1, M. Furman 3, G. Iadorola 1, M. Pivi 2, C. Rivetta 2, G. Rumolo 1, R.
Secondo 1, O. Turgut 2, S. Uemuda 2, J.-L. Vay 3
1 European Organization for Nuclear Research2 SLAC National Accelerator Laboratory
3 Lawrence Berkeley National Laboratory
Work supported by DOE
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 2/27
Outline
i. Simulation models – CMAD, HeadTail, WARP
ii.Feedback system model
iii.Damping the centroid motion
iv.Electron cloud instabilities
v.Damping the intra-bunch motion
vi.Conclusions and outlook
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 3/27
C-MAD, HeadTail, WARP - Models
CMAD HeadTail WARP
Language Fortran C++ Fortran with Python interface
Parallel yes no yes
Optics Smooth or lattice(MAD-X import)
Smooth or lattice (MAD-X import)
Smooth or lattice
PIC 2D FFT 2D FFT AMR (includes space charge)
Binning Constant space or constant charge
Constant space Constant space
Distributions Internal & external Internal & external Internal, external & build-up
Extras IBS, radiation damping, quantum excitation
ZBASE impedance database
Build-up + tracking (strong-strong)
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 4/27
Feedback system implementation
Filter receiver● Pick-up● Cables● Receiver● ADC● Saturation
Processing channel
● FIR-IIR filterswith intrinsic delay
Noise receiver
Filter kicker● DAC● Amplifier● Cables● Kicker● Saturation
Gain
Noise amplifier Excitation
yout
vout
yslice
ykick
yin
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 5/27
Feedback system - specifications
5 tap delay
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 6/27
Feedback system - specifications
5 tap delay
FIR transfer functions (left)
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 7/27
Feedback system - specifications
5 tap delay
FIR transfer functions (left)
Kicker transfer functions (right)
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 8/27
Centroid motion – gain scanBandwidths:200MHz, 500MHz, 700MHz, 1GHz
Perturbation: 2mm initial vertical offset → monitor bunch response
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 9/27
Centroid motion – gain scanBandwidths:200MHz, 500MHz, 700MHz, 1GHz
Perturbation: 2mm initial vertical offset → monitor bunch response
For high gains, the limited (200MHz) bandwidth makes the system become unstable
200 MHz
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 10/27
Centroid motion – gain scanBandwidths:200MHz, 500MHz, 700MHz, 1GHz
Perturbation: 2mm initial vertical offset → monitor bunch response
For high gains, the limited (200MHz) bandwidth makes the system become unstable
For all cases, the bunch response (centroid motion) to the initial perturbation is similar → the systems perform equally well
0 2 4 6 8 10 120
0.5
1
1.5
2
2.5
3
3.5
200 MHz
500 MHz
700 MHz
1000 MHz
Gain [1e-3]
Da
mp
ing
tim
e [m
s]
200 MHz
500 MHz
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 11/27
Comparision CMAD-HeadTail
Perturbation: 2mm initial vertical offset
Gain g ≈ 8.5e-3
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 12/27
ECI – ρe scan
Intensity 1.1e11 ppb
Energy 26 GeV
Emittances [epsx, epsy] 2.8, 2.8 microns
Beta-functions [βx, βy] 42, 42 m
Tunes [Qx, Qy, Qs] 26.130, 26.185, 0.0059
E-cloud region Bends
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 13/27
ECI – ρe scan
Intensity 1.1e11 ppb
Energy 26 GeV
Emittances [epsx, epsy] 2.8, 2.8 microns
Beta-functions [βx, βy] 42, 42 m
Tunes [Qx, Qy, Qs] 26.130, 26.185, 0.0059
E-cloud region Bends
The instability threshold is around ρ
e ≈ 4e11 m-3
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 14/27
ECI – ρe scan
Intensity 1.1e11 ppb
Energy 26 GeV
Emittances [epsx, epsy] 2.8, 2.8 microns
Beta-functions [βx, βy] 42, 42 m
Tunes [Qx, Qy, Qs] 26.130, 26.185, 0.0059
E-cloud region Bends ρe = [1,16] x 1e11 m-3
The instability threshold is around ρ
e ≈ 4e11 m-3
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 15/27
ECI – ρe scan
The instability threshold is around ρ
e ≈ 4e11 m-3
Unstable modes are {0, -1, -2}
Intensity 1.1e11 ppb
Energy 26 GeV
Emittances [epsx, epsy] 2.8, 2.8 microns
Beta-functions [βx, βy] 42, 42 m
Tunes [Qx, Qy, Qs] 26.130, 26.185, 0.0059
E-cloud region Bends ρe = [1,16] x 1e11 m-3
ρe [1e11 m-3]
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 16/27
ECI – ρe ≈ 6e11 m-3
Clear coherent motion above the instability threshold
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 17/27
ECI – ρe ≈ 6e11 m-3
Clear coherent motion above the instability threshold
The mode evolution reveals the presence of predominantly modes {0, -1, -2} (shifted)
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 18/27
Intra-bunch – ρe ≈ 6e11 m-3 – gain scan
Perturbation: electron cloud
Bandwidths:200MHz, 500MHz, 700MHz, 1GHz
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 19/27
Intra-bunch – ρe ≈ 6e11 m-3 – gain scan
Perturbation: electron cloud
Bandwidths:200MHz, 500MHz, 700MHz, 1GHz
For high gains, the limited (200MHz) bandwidth makes the system become unstable
200 MHz
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 20/27
Intra-bunch – ρe ≈ 6e11 m-3 – gain scan
Perturbation: electron cloud
Bandwidths:200MHz, 500MHz, 700MHz, 1GHz
For high gains, the limited (200MHz) bandwidth makes the system become unstable
A gain of 6e-3 appears to damp the ECI
200 MHz
500 MHz
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 21/27
500MHz – ρe scan – gain = 6e-3
Coherent motion is damped within the rangeρ
e = [1,10] x 1e11 m-3
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 22/27
500MHz – ρe scan – gain = 6e-3
Coherent motion is damped within the rangeρ
e = [1,10] x 1e11 m-3
The power in modes{-1,0,1} is effectively diminished
The remaining power appears to be distributed over a wide range of modes
ρe [1e11 m-3]
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 23/27
500MHz – ρe ≈ 6e11 m-3 – gain = 6e-3
Clear damping of the coherent motion
Remaining power is distributed over modes {2,6}
24/27
Feedback power required
Same scale: Low feedback power is required to stabilize the beam in the presence of electron cloud
Feedback ON: no electron cloud Feedback ON: ecloud density 5e11/m3
Kick applied to individual bunch slices by the feedback system
x 1e-5x 1e-5
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 25/27
500MHz – ρe ≈ 14e11 m-3 – gain = 6e-3
Clear re-emerging of the coherent motion
Power is concentrated predominantly in modes {6} (shifted)
Kevin Li ECLOUD'12, 5-9 June 2012, La Biodola, Isola d'Elba 26/27
Conclusions & outlook
Successful implementation of realistic feedback system into multi-particle instability codes
Mode analysis of ECI reveals unstable modes up to mode 2 (for the investigated configuration)
200MHz feedback is insufficient to damp ECI
500MHz feedback provides damping withinfor gains > 6e-3
Study the impact of noise on the feedback effectiveness