PEP-II Lattices. U. Wienands for many others from AD, ARD, NLC. U. Wienands, PEP-II MAC

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Transcription:

PEP-II Lattices U. Wienands for many others from AD, ARD, NLC

PEP-II Lattices Parameters & how we determine them Online Lattice Model Coupling Orbit Control Working point & MIA Lattice Correction Priorities for Run 4

Lattice Parameters HER LER design present design present ßx * (cm) 50 30 50 50 ßy * (cm) 1.5 1.2 1.5 1.1 µx,arc ( ) 60 60 90 90 µy,arc ( ) 60 60 90 90 νx 24.62 24.52 38.57 38.52 νy 23.58 23.58 36.64 36.58 αp 0.00241 0.00240 0.00124 0.00124 ξx n:-43 +2 n:-60 +2 ξy n:-57 +4 n:-70 +2 εx (πnm-r) 48 48 48 30 εy (πnm-r) 2 2 2 1 δp/p 6.1E-4 6.1E-4 7.7E-4 6.2E-4 σx * (µm) 155 117 155 122 σy * (µm) 5.5 5 5.5 3.3 τx (ms) 37 37 61 72 τs (ms) 19 19 30 36 No wiggler!

Lattice-function measurement Measure 1024-turn phase advance/bpm Compare to online model Calculate ß, a relative to the model used. Method pioneered at CERN (Castro-Garcia) Worked well for HER, not well for LER with 90 /cell. SLAC extension for 90 /BPM (M. Donald) Now implemented online (Zelazny, Himel)

Online beta functions LER X LER Y

HER β x at waist Derived from supporttube BPMs M.H. Donald

Dispersion (LER, vertical) L 6.3E33

Dispersion (HER, vertical) L 6.3E33

Online Lattice Model To model PEP rings, need too include orbits New models created from the design Running on dedicated Linux computer networked to VMS Can use saved magnet configurations and orbits Can put results back into online (SCP) DB (J. Turner, M. Woodley, M. Donald, U.W.) Compare to phase-advance measurements Local fit using model as a beam line Can we identify magnet errors?

HER Model/Actual Settings under development M. Woodley β y η y Orbit x Orbit y

Coupling Global coupling easily corrected to 100 Hz Usually not the highest luminosity Operationally, 400 1000 Hz is best Measured using closest-tune approach Have also scanned beam height Local coupling measured by orbit coupling Global orbit wave in one plane couples into other plane Used originally to tune the solenoid compensation (Y. Cai)

Coupling Resonance Scan (HER) Beam height (mm) 2.50 2.00 1.50 Width: 93 Hz Reswidth:0.000689328 1.00 0.0000 0.0050 0.0100 0.0150 nu

Orbits Relatively large orbit offsets HER absolute Golden orbits, known to give good lumi. Relatively large unknown BPM offsets in IR 2 In the LER, affects coupling

Orbit Control Need to maintain collisions IPXY, centers x & y, also aligns the yp Dither feedback acting on luminosity signal Biggest source of drift are the IP quads => HERO, LERO, acting on one X and one Y corr. in IR Biggest concern is at the local sextupoles => HSXT, LSXT loops in Arcs 1/3 Want orbit stable at TFB pickups HTFB, LTFB loops in IR 4

Orbit Control (cont d) Main concern with these loops: crosstalk HERO, LERO have global effect Directly interfere with IPXY as IP not maintained Other loops nominally closed bumps. New, global auto-steering loop: GOF SVD steer each ring about every 10 min. IP transparent to avoid losing collisions Avoid interference with other f/b loops Watch corrector and energy creep!

Orbit shift after 1 week With GOF running Some locations are subject to tuning (e.g. in Arc-1, Arc-3 sexts, collim.). General shift requires IR steer every few days

Energy drift due to GOF Energy can be reset by dialing in a dispersionlike corrector pattern

IR 2 Surveying vs HERO/LERO A. Seryi, S. Ecklund

Measured IP Beam Sizes Measured by beam-beam scans ( scans) Diagonal scans also give average IP roll (F.-J. Decker) x = 117µm y = 6.8µm

Change of Working Point(s) Lower LER ν x to 0.52 0.53 Strong ß beat prevented luminosity gain Fixed using MIA technique LER tune-scan simulation (I. Reichel)

LER tune move (cont d) LER move successful Using MIA technique to control ß-function beating in x Essential to move HER x tune as well!! But this causes large HER beta beat( 2:1) which lowered HER ß*x to 30 cm. Need to use MIA to fix HER ß beat Want to maintain ß* at 25 30 cm And also maintain state of coupling.

Tune Scans (B-B Simulation) LER-only (I. Reichel) LER & HER equal tunes

Spectra in Collision LER HER

After moving tune LER ß at low ν x ß x (m) 200 150 100 50 0 blk: ß measured, red: ß model 500 1000 1500 2000 Distance (m) After ß fix ß_x (m) 200 150 100 50 0 blk: ß measured, red: ß model 500 1000 1500 2000 Distance (m)

MIA Analysis & Correction Find model of extant lattice from 1024-turn BPM data ( Virtual Machine ). Yiton Yan Fit to wanted machine finding magnet changes Measure changed machine to verify

Machine Acceptance Sufficient beam life times (at production current) suggest good acceptance: HER: 15 hrs single beam, 7 hrs in collision beam-gas (bremsstrahlung) & beam-beam limited LER: 3 4 hrs single beam, 1.5 3 hrs in collision Touschek limited, some beam-beam, Momentum acceptance: Touschek expt: LER: 0.7%, as design HER: not known but likely as good or better.

Lattice Priorities for Run 4 Have an accurate lattice model will make lattice MD more efficient Fix our beta beats (mostly HER x, now) Re-commission ORM to aid in diagnosis of mag. errors Control and lower β as far as possible aim for β y = 0.9 cm, β x 28 cm Eventually will be aperture or chromaticity limited Better stabilize & control our orbits Control coupling in the IR & at the IP D. Sagan/Cornell here in two weeks.

Lattice Priorities (cont d) Be able to taylor the beam emittance Important when beam-current limited I d like to characterize the lattice 1/week Will cost about one hour of program time, β (ph. Adv.), η, ν, Yunhai orbits, coupling The more we ask from the machine, the tighter we will have to control our lattices.