Integrated ATF2 Dynamic Tuning Simulations Glen White, LAL/SLAC ATF2 Software Workshop June 2008 Simulation overview. Tuning for 37nm IP vertical beam.

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Presentation transcript:

Integrated ATF2 Dynamic Tuning Simulations Glen White, LAL/SLAC ATF2 Software Workshop June 2008 Simulation overview. Tuning for 37nm IP vertical beam size. Dynamic stability. Further work and FS integration.

Oct 9, 2007Glen White2 Overview  Make a detailed dynamic simulation of ATF2 alignment and tuning steps to assess feasibility of getting and maintaining ~37nm spot size when considering all error sources.  All simulations in Matlab with Lucretia.  Try and include all tuning steps after initial commissioning (ie beam gets to end of beamline).  Review further work and steps towards Flight Simulator integration.

Oct 9, 2007Glen White3 Error Parameters  Errors are normally distributed with mean=ref. orbit and quoted standard deviations.  EXT BPM alignment not directly modeled yet, assume 10um quad-bpm alignment here.  Model for SM measurement: mean spot size from 90 consecutive pulses +/- 2nm RMS error.  Poisson-calculated multipole errors in FFS dipoles.  Measured final quad doublet errors available, not in simulation yet 2nm (+ dyn. Err cont.)Shintake Monitor Resolution 20 (FFS)/11 (EXT) bitPower supply resolution (not included in this simulation as shown) 100 nmBPM resolutions 50 nm Mover step size (x & y)‏ 1e-4 syst. + 1e-4 randomdB/B for Quad, Sexts 30 umInitial BPM-magnet field center alignment 300 uradQuad, Sext / Bend roll alignment 200 umx/y/z alignment errors

Oct 9, 2007Glen White4 Dynamic Errors  RMS pulse-pulse errors: Component jitter: 25 nm. Energy error: 1E-4. Ring extraction jitter: 0.1 sigma (x,x’,y,y’).  Pulse-pulse feedback using FFS FB + EXT steering algorithm.  Ground motion: use modified model K from ATF measurements: Ground motion ATF. Tentative version K model 'Parameter A of the ATL law, A [m**2/m/s] ' E-17 'Parameter B of the PWK, B [m**2/s**3] ' E-18 'Frequency of 1-st peak in PWK, f1 [Hz] ' E-01 'Amplitude of 1-st peak in PWK, a1 [m**2/Hz] ' E E-11 'Width of 1-st peak in PWK, d1 [1] ' E+00 'Velocity of 1-st peak in PWK, v1 [m/s] ' E E+03 'Frequency of 2-nd peak in PWK, f2 [Hz] ' E+00 'Amplitude of 2-nd peak in PWK, a2 [m**2/Hz] ' E E-15 'Width of 2-nd peak in PWK, d2 [1] ' E+00 'Velocity of 2-nd peak in PWK, v2 [m/s] ' E E+02 'Frequency of 3-rd peak in PWK, f3 [Hz] ' E+00 'Amplitude of 3-rd peak in PWK, a3 [m**2/Hz] ' E E-17 'Width of 3-rd peak in PWK, d3 [1] ' E+00 'Velocity of 3-rd peak in PWK, v3 [m/s] ' E E+02

Oct 9, 2007Glen White5 Pulse-Pulse Feedback  Use pulse-pulse feedback to get initial beam orbit through EXT and FFS and maintain orbit when GM drifts added.  FFS FB/EXT FB gain ration 10/1 (orbit stability most important in FFS).  EXT feedback “least-squares matrix-inversion” steering using all correction magnets (ZV*X & ZH*X) and quad BPMs.  FFS feedback 2 kicker-BPM pairs for x & y feedback at 90-degree phase separations.

Oct 9, 2007July 18,20076 IP IP phase FD phase IP phase FD phase IP phase FD phase IP phase FD phase IP phase FD phase ZV11X ZV1FF QBPM7F F nBPM 3 ZH10 X ZH1F F ML1FF QBPM9F F ZH ZV BPM

Oct 9, 2007July 18, µm 0.4 µm µm 7.9 µm ZH BPM ZV BPM

Oct 9, 2007Glen White8 IP Beamsize Measurement  Shintake monitor measurement range 35nm – 350nm.  Wirescanner for >1 micron waist sizes.  Between 350nm and ~1um, 'Honda Monitor'.  In this simulation, just use Shintake monitor resolution- when using sextupole knobs, arrive in SM range quickly (1 or 2 iterations usually).

Oct 9, 2007Glen White9 Tuning Procedure Overview  Use EXT correctors + BPMs (EXT FB) to get orbit through EXT.  Use FFS FB to get beam through FFS.  Correct Dy/Dy' in EXT using skew-quad sum knob.  Correct coupling in EXT using coupling correction system.  Use FFS FB for launch into FFS.  FFS Quad BPM alignment using quad shunting with movers.  FFS Quad mover-based BBA.  FFS Sext BPM alignment using Sext movers and downstream BPMs.  Sextupole mover tuning knobs to get final spot size Vertical IP dispersion and Waist coupling Higher order terms collectively through Sext rolls + dK.  Also use EXT skew-quads to tune other coupling terms.

Oct 9, 2007Glen White10 Simulation Notes  Ideal simulation includes tracking every bunch, including inter-pulse jitter effects on IP size measurement (90 pulses per measurement).  This takes a LONG time with macro-particle bunches.  Simulation includes GM effects (ie. 90 / 1.5Hz GM added for every IP size measurement).  Effect of fast jitter during 90 pulse IP size measurement is modeled as effective degradation of IP measurement resolution.  For dynamic errors studied here, pulse-pulse jitter effects add 1.3nm (in quadrature) to 2nm SM measurement ( giving res. ~2.4nm).

Oct 9, 2007Glen White11 Beam Model  Lucretia beam models: 'Sparse' := 2 nd order moment tracking in transverse 'Macro-particle':= better for handling higher-order effects- non-Gaussian beam. Slower.  Tracking through perfect lattice (100 generated bunches)‏ Sparse beam gives 35.0 nm IP beam non-Gaussian, higher-order effects important as well as measurement of beam size.

Oct 9, 2007Glen White12 EXT Tuning Results  With an error-free FFS, tune EXT with 10K and 80K macro-particle beams (100 seeds).  Median results the same.  Probably ok to do full tuning with 10K bunch with same perfect-lattice performance as the mean 100K-case.  Use 10K bunch for simulation results shown in this talk.

Oct 9, 2007Glen White13 Quad & Sext BPM Alignment  RMS alignment of Magnet field centre – electrical centre of magnet BPMs (100 seeds).  Blue = x Red = y.

Oct 9, 2007Glen White14 Beamsize after BBA  IP waist size before sextupole FFS tuning knobs applied (100 seeds).

Oct 9, 2007Glen White15 Multi-Knob Tuning Results  IP spot size vs. # of pulses (assuming 90 pulses per IP size measurement).  Fast convergence <100nm (after fixing waist + dispersion). ~ 144 Hours Static Simulation

Oct 9, 2007Glen White16 Best Spot Size Achieved  Min IP waist size achieved vs. pulse #  Mean and +/- 1 sigma plotted from 100 seeds.  Red = static, blue = dynamic.

Oct 9, 2007Glen White17 Tuning Results

Oct 9, 2007Glen White18 Final Quad Mover Positions  Position of Quad Magnet Movers after tuning.  x/y moves ~<2mm possible, but have to take into account map of x,y,roll phase space.  Need to check don't try to move outside this phase space.

Oct 9, 2007Glen White19 Final Sextupole Mover Positions  x/y positions of Sext movers after tuning.

Oct 9, 2007Glen White20 Final Sextupole Mover Rolls  Final roll positions of sextupole movers.

Oct 9, 2007Glen White21

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Oct 9, 2007Glen White26 Most Important Jitter Sources  Final Focus Magnet vibrations and jitter of EXT corrector magnetic field  Expected jitter from 'Nominal' Parameters = ~35 nm RMS pulse-pulse

Oct 9, 2007Glen White27 Jitter Source Concerns  From Shintake BSM group: 2nm IP measurement resolution with ~30nm jitter between laser fringe and beam  10nm expected jitter from laser  BUT expect >~35nm for beam from jitter sources studied here... Need IP beam- based multi-bunch feedback?  Only 11-bit corrector PS's in EXT line? 1-bit of noise= 1e-3 fluctuation of corrector, not 1e-4 as in 'nominal' jitter source set simulated here. Means 110nm IP jitter!

Oct 9, 2007Glen White28 BSM Measurement Simulation

Oct 9, 2007Glen White29 Further Work / Conversion of Code to FS  EXT BBA simulation needed  FFS BBA Simulation and FS code exists for Quad shunting Simulate and compare ballistic alignment/DFS  EXT Disp. Correction Effects of DR freq. ramp other than E sweep? Need EPICS interface to DR freq. Ramp to include in FS.  EXT/FFS Steering/ Feedback Need global Feedback FS code (all feedbacks)

Oct 9, 2007Glen White30 Further Work / Conversion of Code to FS  EXT coupling correction. Add wirescanner errors to simulation Need EPICS wirescanner interface for inclusion into FS.  Add more realistic constraints to sim Respect apertures Radiation monitoring during BBA.‏  Model Effects on tuning of jitter sources with medium-length timescales ~few mins drift of water temp etc

Oct 9, 2007Glen White31 Further Work / Conversion of Code to FS  Final Tuning Procedure Need to improve on simulations (method)- look at other methods in integrated simulation environment, proper comparison of different techniques... Better % of seeds closer to tuning goal, faster convergence rate (better tuning algorithm) Understand and include BSM measurement analysis Alter procedures to fix cases where magnet movers go out of range Jitter conditions look too bad? FS inclusion needs IP monitors in EPICS

Oct 9, 2007Glen White32 Further Work / Conversion of Code to FS  IP multi-bunch feedback to mitigate IP beam jitter for BSM measurement Feasibility study When would hardware to do this be available Who could do this?