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Vertical Emittance Tuning at the Australian Synchrotron Light Source Rohan Dowd Presented by Eugene Tan Overview Machine overview LOCO method and minimisation technique Minimisation results and Measurements Sextupole


  1. Vertical Emittance Tuning at the Australian Synchrotron Light Source Rohan Dowd Presented by Eugene Tan

  2. Overview • Machine overview • LOCO method and minimisation technique • Minimisation results and Measurements • Sextupole alignment measurements • Conclusion ICFA - Low Emittance Ring Workshop 3-5 October 2011

  3. Australian Synchrotron Light Source Overview • Double bend lattice • 14 fold symmetric • Gradient dipoles • Corrector and skew quad coils on sextupoles. • Independent power supplies for all multipoles. • Storage Ring Parameters Energy 3 GeV Circumference 216 m RF Frequency 499.654 MHz Peak RF Voltage 3.0 MV Current 200 mA Betatron Tune (h/v) 13.3/5.2 Momentum Compaction 0.002 ε x (nominal) 10.4 nm∙rad ICFA - Low Emittance Ring Workshop 3-5 October 2011

  4. LOCO method • LOCO – Linear Optics from Closed Orbits. • Adjusts the linear optics in the model to fit the real machine data • Model response matrix – Machine response matrix = Error • Minimise error by adjusting the model ‘fit parameters’ • Fit Parameters normally include: – BPM/Corrector gains and coupling – Corrector gains and coupling – Quadrupole strengths – Skew Quadrupole strengths • We fit skew quadrupole components in all multipole magnets in our model lattice to represent rolls and misalignments. ICFA - Low Emittance Ring Workshop 3-5 October 2011

  5. LOCO Outputs Verified from attenuation measurements for the BPM. Outputs: • BPM Gains + Couplings • Skew components • Quad Strengths • Corrector gains/tilts From these outputs we can calibrate the model and calculate skew corrections needed to Fits to varying machine coupling states (0.01- adjust coupling 17% coupling) Consistent BPM/corrector coupling results for differing machine coupling settings – LOCO is not attributing the machine coupling to BPM/corrector coupling Fits to identical machine coupling (10 samples) ICFA - Low Emittance Ring Workshop 3-5 October 2011

  6. Emittance Coupling minimisation • Emittance coupling ( ε y / ε x ) calculated from LOCO Calibrated model. • Minimisation algorithm used to adjust skew quads to desired emittance coupling. • Emittance coupling can be adjusted to arbitrary amounts with this method. Set Coupling LOCO Measured Calculated ε y (pm) Coupling 0.0% 0.01% 1.0 0.1% 0.12% 12.2 0.2% 0.23% 23.5 0.3% 0.33% 33.7 0.4% 0.43% 43.9 0.5% 0.54% 55.1 0.6% 0.64% 65.3 0.7% 0.74% 75.5 0.8% 0.84% 85.7 0.9% 0.92% 93.8 1.0% 1.04% 106.1 Phys. Rev. ST Accel Beams, 14, 012804 (2011)

  7. Touschek Lifetime vs RF • By taking single bunch lifetime over extended period the Touschek component of the lifetime can be extracted.      2 1 Nr c D ( )      e max x , ,          2 3   8 z max x y x      u u 3  e ln( u ) 1  e                  D ( ) e du ( 3 ln( ) 2 ) du       2 2 u 2 u 2 di i i    dt a b 1  a i be  0 i ( t ) 1    a b i a ( 1 e ) 0 ICFA - Low Emittance Ring Workshop 3-5 October 2011

  8. Touschek Lifetime vs RF • Touschek component will also change with RF voltage. • 2.1% energy acceptance (measured) • Curve fit by varying ε y / ε x , other values fixed. • Blue curve fit corresponds to ε y = 1.24 pm Set ε y / ε x Fitted ε y / ε x ε y (pm) (%) (%) 0.01 0.012 ± 0.003 1.2 ± 0.3 0.06 0.043 ± 0.013 4.5 ± 1.3 0.10 0.093 ± 0.025 9.4 ± 2.6 ICFA - Low Emittance Ring Workshop 3-5 October 2011

  9. Tune Crossing Results LOCO Model ε y (pm) η y Component (pm) Betatron Coupling Total Measured ε y Model – Measured Component (pm) (pm) (pm) 92.31 ± 2.77 2.24 ± 0.09 86.90 ± 2.65 89.55 ± 2.65 2.76 ± 3.83 76.30 ± 2.23 2.96 ± 0.12 76.50 ± 2.14 78.64 ± 2.14 2.34 ± 3.09 41.41 ± 1.24 1.73 ± 0.07 40.39 ± 1.84 42.23 ± 1.84 0.82 ± 2.22 22.75 ± 0.68 2.04 ± 0.08 19.69 ± 1.33 21.72 ± 1.33 1.03 ± 1.49 12.75 ± 0.38 2.14 ± 0.09 10.71± 1.02 12.85 ± 1.02 0.10 ± 1.09 7.55 ± 0.23 1.73 ± 0.07 5.41 ± 0.71 7.14 ± 0.71 0.41 ± 0.75 1.05 ± 0.03 0.73 ± 0.09 0.59 ± 0.30 1.32 ± 0.31 0.27 ± 0.31 ICFA - Low Emittance Ring Workshop 3-5 October 2011

  10. How to improve? • With current correction scheme we are stuck at 1-2 pm. • Instead of correcting for misalignments, lets eliminate them. • Recent ring alignments have made the coupling worse! • Need to measure them independently – Beam based method ICFA - Low Emittance Ring Workshop 3-5 October 2011

  11. Sextupole offsets • Shunt each sextupole magnet family to different strengths and take a response matrix at each point • Perform LOCO analysis and fit skew quadrupole terms to each sextupole. • Gradient of skew field vs sextupole field gives vertical offset. ICFA - Low Emittance Ring Workshop 3-5 October 2011

  12. Sextupole Offset Results • Average offset: 70 microns • Systematic alignment effect? ICFA - Low Emittance Ring Workshop 3-5 October 2011

  13. Cross Checks Applied BPM Offset Measure Mean Beam Difference from zero Offset +125 234.6 ± 10.6 128.7 ± 18.8 +75 167.7 ± 16.5 61.8 ± 22.6 0 105.9 ± 15.5 0 -75 33.1 ± 17.8 -72.8 ± 23.6 -125 -16.1 ± 21.6 -122 ± 26.6 Magnet Original Offset Applied Shim New Offset Delta offset ( μ m) ( μ m) ( μ m) ( μ m) Sector 9 SFB -108.4 ± 44.6 150 -249.3 ± 7.2 140.9 ± 45.2 Sector 11 SFB -56.7 ± 10.0 100 -120.4 ± 56.0 -63.4 ± 57.4 Sector 9 SDA -14.6 ± 9.9 100 -118.3 ± 8.3 -103.7 ± 14.1 Cross checks show that amplitude of offset is correct and individual magnets can be adjusted accurately. ICFA - Low Emittance Ring Workshop 3-5 October 2011

  14. Sextupole Realignment – latest results Re-aligned section (girder #16-21) now has much lower offsets. Simulated minimal vertical emittance has reduced from 1pm to 0.7 pm. ICFA - Low Emittance Ring Workshop 3-5 October 2011

  15. Conclusions • ε y of 1.3 pm.rad achieved through LOCO based minimisation. • We have developed tools to accurately measure sextupole misalignments and eliminate them. • Aim to have all sextupoles realigned by end of year and expect to reach < 1 pm emittance • Also working on an inexpensive way to increase available skew correctors ICFA - Low Emittance Ring Workshop 3-5 October 2011

  16. Thank you ICFA - Low Emittance Ring Workshop 3-5 October 2011

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