Effect of alignment errors on Touschek lifetime, dynamic apertures and injection efficiency S.M. Liuzzo, (Post-Doc, ESRF), 10-13 march 2015, CAoPAC Workshop, GSI, Darmstadt OUTLINE The influence of errors on the ESRF upgrade lattice will be presented: - Uncorrected errors - BPM and correctors locations in the ESRF cell - Corrections scheme - Strategies for error tolerance definitions: comparable tables and tolerable errors list - Random alignment errors - Multipole errors - Long range and survey errors - Effects on beamlines Page 2 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo MISALIGNMENTS Real accelerators are not perfectly aligned. Unwanted fields are present in the lattice: Quadrupole Sextupole Sextupole Page 3 Misaligned Quadrupole Quadrupole Dipole Vertically Misaligned Sextupole Sextupole Skew Quadrupole Dipole Horizontally Misaligned Sextupole Sextupole Quadrupole Dipole l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo NUMBER OF TURNS VS ERROR AMPLITUDE WITHOUT CORRECTION On axis Increasing the vertical displacement of quadrupoles introduces vertical orbit and coupling. Off axis For an uncorrected lattice a beam injected on axis can perform 100 turns with 50 um vertical quadrupole offsets A beam injected off axis, can perform only 10 turns for the same error rms. Page 4 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo NEEDS AND CHALLENGES FOR OPTICS CORRECTION: CORRECTORS AND BPM Correctors in all sextupoles plus 3 separated correctors All magnets have independent power supplies 10 BPM 9 correctors, horizontal, vertical and skew quadrupole in all sextupoles and 3 dedicated correctors 16 quadrupoles DL Page 5 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo DL DQ DQ EXAMPLE OF CORRECTION OF RANDOM ERRORS Simulation of the whole correction sequence, from transfer line to ORM* fit. - Find a closed orbit correcting open trajectories - Correct orbit - Create lattice error model fitting ‘measured’ RM (partial, 14/288 cor.) ORMerr = [ ORM/K ] * Kfit - Compute Resonance Driving Terms and correct simultaneously normal and skew quadrupole RDT and dispersion After tuning Current ESRF X [mm] 160(675) 116 61 Y [mm] 111(250) 58 70 Dx-Dx0 [m] 0.017 0.001 0.028 Dy [m] 0.002 0.0002 0.002 b-beating x [%] 26.2 0.7 4.9 b-beating y [%] 26.5 0.8 3.3 Tune x [.21] 0.208 0.21 0.44 Tune y [.34] 0.336 0.34 0.39 Q’x [6] 6.328 6.00 3.89 Q’y [4] 3.971 4.00 6.92 - Fix tune and chromaticity ex [134.7 pmrad] 250.4 134.7 4099 - Iterate a few times ey [ 0.04 pmrad] 2.2 0.18 3.123 *Orbit Response Matrix Page 6 Closed orbit only l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo Corrector strengths [rad/L] INITIAL OPEN TRAJECTORY CORRECTION Orbit corrector # Page 7 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo DISPERSION AND BETA BEATING CORRECTION (NORMAL AND SKEW QUAD.) Page 8 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo DEFINITION OF TOLERABLE ERRORS To define tolerable errors, we need a deterministic procedure, applicable to any lattice, and comparable. 1. Compute relevant parameters vs interesting error sources 2. Define accepted threshold for each parameter 3. Chose tolerable error has the minimum value that exceeded a threshold 4. Consider combinations of errors For the ESRF upgrade lattice some additional care in the error definitions is also required: Page 9 • for magnets modeled in more parts: longitudinal gradient dipoles, combined function magnets, sextupoles. • distinguish between errors and correction in quadrupoles. • Dipole errors do not change the reference trajectory. l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo LIFTIME AND DYNAMIC APERTURES VS ERROR SOURCES 17h DA=-10mm Lifetime = 10h 10h A CLUSTER is crucial for this analysis. Each error set to analyze requires 1CPUx4h Page 10 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo COMPARABLE TOLERANCE TABLE • • • • • Page 11 DQ (combined function dipoles) behave as quadrupoles concerning errors. Evident the impact on vertical dispersion compared to the other quadrupoles (defocussing quadrupoles). Quadrupoles have large impact on orbit and horizontal dispersion, also in this case, lifetime and DA are strongly affected. QF6 and QF8 are dominant. Sextupoles have the largest impact on DA, they are also the strongest source of beta-beating and emittance as expected. Octupoles influence is limited compared to quadrupole and sextupoles, nevertheless they do have an impact on DA. Their effect on lifetime is very small. Rotations up to 100urad have impact on the various parameters but limited. l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo COMPARABLE TOLERANCE TABLE • This table provides a deterministic way to compare error impact on lattices. • It is used also to asses the performances of correction schemes and correction algorithms • Further reduction of this data is needed to provide a tolerance table. Page 12 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo DEFINITION OF A LIST OF TOLERABLE ERRORS Compare magnet groups for the same error beta beating = 1% Compare error sources for the same magnet group Hor. Disp. = 1mm Tolerated errors Page 13 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo TOLERABLE RANDOM ERRORS Each error, on each magnet family, is studied individually looking at the dependence of DA, lifetime, emittances and all relevant parameters vs error amplitude. Required: DX DY DS DPSI DK mm mm mm mrad 10^-4 >100 >100 1000 500 10 DQ, QF[68] 70 50 500 200 5 Q[DF][1-5] 100 85 500 500 5 SFD 70 50 500 1000 35 OF 100 100 500 1000 DL Sextupoles and high gradient quadrupoles are the most relevant limitations, nevertheless, this alignment specifications are currently achievable. (DX=DY=60mm, 84 mm between two magnets). Page 14 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo LIFETIME, DYNAMIC APERTURE AND INJECTION EFFICIENCY With the dedicated injection section and an appropriate injected beam the upgrade lattice has injection efficiency of 98+/-1% (average of 10 seeds), With a lifetime of 21+/-1 h (average of 10 seeds), 43 h without errors. septum Injected beam Kicked beam This figure uses as errors the table above. It might be used as the standard candle for the lattice accompanied by lifetime and injection efficiency Stored beam averages. Injection bump Page 15 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo MULTIPOLE ERRORS Page 16 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo LAMINATED MAGNET MULTIPOLE ERRORS: EFFECT ON DYNAMIC APERTURE D.A.: 10.3+/-0.5 mm L.T. : 21.3 +/- 1 h I.E. : 98% Page 17 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo D.A.: 10.7+/-0.6 mm L.T. : 21.3 +/- 1 h I.E. : 98% CORRECTOR MULTIPOLES Bx(x)/B0 G(x)/G0 Page 18 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo By(x)/B0 At every update of the correctors values this multipoles must be recomputed. CORRECTOR MULTIPOLES + STANDARD ERRORS D.A.: 10.3+/-0.5 mm L.T. : 21.3 +/- 1 h I.E. (30nm,round) : 98% Page 19 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo D.A.: 9.8+/-0.7 mm L.T. : 21.4+/-1.2 h I.E. (30nm,round) :97+/-2 % LONG RANGE ERRORS nominal measured storage ring survey data Page 20 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo simulated 1st harmonic, ERROR AMPLITUDE GIVING 30UM ORBIT AFTER CORRECTION VS WAVELENGTH Amplitude is X, Y and rotation about s (rad) simultaneously Simulations performed on the OAR asd cluster, about 8h-600cpu Page 21 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo DYNAMIC APERTURE AND LIFETIME Lifetime: 16.6h range:[16.4 17.1] nominal measured -10mm (-8.1mm @injection) Page 22 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo CURRENT ESRF SURVEY X-ray beam direction is strongly influenced by the position of the storage ring and orbit distortion. Page 23 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo X-RAY BEAM POSITION AT ID (60 METERS) All ID are assumed to be at 60m from the source. The position of the beam after 60m is very similar for ESRF and S28A considering the current survey measurement. The position if the ring was aligned on the reference circumference would be about (0,0) for al ID. Current (simulated) position of the X-ray at the beamline Page 24 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo position of the X-ray at the beamline for S28A on the same survey CONCLUSIONS ESRF lattice sensitivity to lattice errors has been shown A complete correction scheme is used to deduce the lattice parameters after correction Random alignment errors are studied to determine a tolerable errors table Long range errors and survey errors are also analyzed, and the impact of the alignment on the beamlines positions is considered. Page 25 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo THANK YOU FOR YOUR ATTENTION! Page 26 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo ALIGNMENT ERRORS DEFINITION IN THE SIMULATIONS Notice: - longitudinal displacement for dipoles is not trivial - Everything respect to the nominal beam trajectory. DS R q Page 27 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo ORBIT CORRECTOR STRENGTHS DISTRIBUTION Vertical Horizontal The central vertical corrector is the strongest. Solutions are under study to reduce its force. This may require a larger corrector, only H-V, or tighter error tolerances. Page 28 H corrector V corrector Required 0.6 mrad 0.78 mrad (SH2 only!) 0.2 T Magnet design 0.6 mrad 0.3 mrad l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo Skew quadrupole 0.43 T DIPOLE FIELDS ERRORS (CONSTANT FIELD INTEGRAL) Page 29 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo ONLY DIPOLE FIELD VARIATION D.A.: 12.4 mm (no errors) L.T. : 43.1 h (no errors) I.E. (30nm,round) : 100% Page 30 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo D.A.: 12.1 +/-0.1 mm L.T. : 40.2 +/- 0.3 h I.E. (30nm,round) : 100% ESRF LATTICE CELL Page 31 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo COIL CURRENTS IN SEXTUPOLE CORRECTION COILS, 10 ERROR SEEDS PS1 1 PS4 6 PS3 Page 32 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo PS2 COIL CURRENTS IN SH DEDICATED CORRECTORS, 10 ERROR SEEDS PS2 PS1 PS3 3 5 2 4 1 Page 33 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo PARAMETERS OF INTEREST VERSUS ERRORS IN SPECIFIC MAGNET FAMILIES 40 instead of 10 seeds, (no Page 34 Horizontal dispersion variation Horizontal emittance variation DA computation) l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo Errors ranges listed in legend SUMMARY TABLE OF ERROR VALUES TO ACHIEVE A GIVEN DISTORTION Example: 28 um of Quadrupole displacements to generate 50um of orbit rms Page 35 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo THRESHOLD CROSSING ERROR VALUES. THRESHOLD @ 9.5 MM DA Overall improvement compared to previously used correction algorithm Page 36 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo Less influence on emittances DETAIL FOR EACH FAMILY Page 37 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo DETAIL ON X-Y DISPLACEMENT FOR EACH FAMILY, 10 ERROR SEEDS DQ1, QF6 and QF8 are the most sensitive to x-y misalignment. Page 38 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo DETAIL ON DPSI FOR EACH FAMILY, 10 ERROR SEEDS DQ1, QF6 and QF8 are the most sensitive to Rotations about the s-axis. Page 39 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo GIRDER ERRORS Girder displacements and rotations Girder displacements and rotations + random errors Quad. and Sext. 4 girders, BPMs are moved with the girder. Page 40 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo GIRDER ERRORS Hor. DA @ QFI, X0.81 to scale at S3, 8mm required at S3, 10mm accepted at QFI 17h 10h Page 41 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo (g) Stands for girder errors, no (g), are quadrupole and sextupole individual misalignments SUMMARY TABLE OF GIRDER ERRORS (g) Stands for girder errors, no g, are quadrupole and sextupole individual misalignments Page 42 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo SEXTUPOLAR RESONANT DRIVING TERMS AFTER CORRECTION Sextupolar RDT no errors Sextupolar RDT with errors Sextupolar RDT after optics correction Page 43 l CAoPAC Workshop l GSI, Darmstadt 10-13 March 2015 l S.M.Liuzzo The use of sextupole independent power supplies will allow to recover also the residual distortion. Work is in progress (N.Carmignani, A.Franchi). More details in Andrea Franchi’s Talk. Many other techniques will be applied and are under study to improve the optics correction, in particular focusing on the correction of off energy beam dynamics and resonant driving terms.