1. 24.09.07 ATF2 meeting LAPP; David Urner 1 David Urner Paul Coe Matthew Warden Armin Reichold Geoffrey Rayner MPhys alumnus MONALISA Monitoring, Alignment & Stabilisation with high Accuracy

2. 24.09.07 ATF2 meeting LAPP; David Urner 2 Compact Straightness Monitor CSM 2-dim sketch (3d requires second lateral measurement ) Use mechanical stability of small platforms A&B. Use multiple lines to cancel systematic effects Resolution scales aproximately with H/L H=~10cm L = as needed A A B

3. 24.09.07 ATF2 meeting LAPP; David Urner 3 FSI: Frequency Scanning Interferometry

4. 24.09.07 ATF2 meeting LAPP; David Urner 4 Progress in 06 / 07 Hardware Built novel Interferometer designs Pioneered new phase measurement techniques Still making vacuum vessel to demonstrate nm precision Tested compact launch optics Software Developed novel phase analysis technique Collaborated with LiCAS on OO analysis package Developed binary file format for data handling users MonAliSA, LiCAS and ATLAS (FSI)... Available in Java, C and LabVIEW

5. 24.09.07 ATF2 meeting LAPP; David Urner 5 Reference Interferometer Both interferometers have same mirror sweep Interferometers cross check step size and other systematics If one is very short and one quite long, uneven laser tuning can be more easily followed Parallel s Piezo Swept mirror

6. 24.09.07 ATF2 meeting LAPP; David Urner 6 Parallel Michelson interferometers built and tested Installed continuous thermometer readout system Calibration studies this autumn Parallel Reference Interferometer

7. 24.09.07 ATF2 meeting LAPP; David Urner 7 Multi-fibre read out (compact launch) Fixed frequency laser (FFI) Same interferometer can be used for FSI Test shown here with moving mirror First stationary mirror test : - resolution 5 nm demonstrated - to be improved with vaccuum - and laser frequency stabilisation - temperature and pressure dependence look reasonable FFI: Fixed Frequency Interferometry (OPD 400mm)

8. 24.09.07 ATF2 meeting LAPP; David Urner 8 Multi-fibre read out (compact launch) Fixed frequency laser (FFI) Same interferometer can be used for FSI Test shown here with moving mirror First stationary mirror test : - resolution 5 nm demonstrated - to be improved with vaccuum - and laser frequency stabilisation - temperature and pressure dependence look reasonable Time (hours) Displacement /  m Displacement / nm  =4.5nm FFI: Fixed Frequency Interferometry (OPD 400mm)

9. 24.09.07 ATF2 meeting LAPP; David Urner 9 Multi-fibre read out (compact launch) Fixed frequency laser (FFI) Same interferometer can be used for FSI Test shown here with moving mirror First stationary mirror test : - resolution 5 nm demonstrated - to be improved with vaccuum - and laser frequency stabilisation - temperature and pressure dependence look reasonable Time (hours) Displacement /  m Time (hours) Displacement /  m Displacement / nm  =4.5nm FFI: Fixed Frequency Interferometry (OPD 400mm)

10. 24.09.07 ATF2 meeting LAPP; David Urner 10  =750nm Multi-fibre read out (compact launch) Fixed frequency laser (FFI) Same interferometer can be used for FSI Test shown here with moving mirror First stationary mirror test : - resolution 5 nm demonstrated - to be improved with vaccuum - and laser frequency stabilisation - temperature and pressure dependence look reasonable  =750nm  =70nm Add box to reduce air turbulence FSI:Frequency Scanning Interferometry (OPD 400mm)

11. 24.09.07 ATF2 meeting LAPP; David Urner 11 Ellipse fitting phase extraction Novel technique for multi-fibre phase readout Signals from 2 fibres Normalise onto unit circle Phase angle

12. 24.09.07 ATF2 meeting LAPP; David Urner 12 Setup at ATF2 Shintake monitor table QD0 ATF2 Beamline Goal: Prove we don’t induce vibrations onto Shintake monitor Problem: No room for wings that are required to get necessary stiffness Possible solutions: -Attach to QD0 support table -Cross brace between Shintake table and QD0 support table 79 Hz mode What is the gap between QD0 support table and Shintake Monitor?

13. 24.09.07 ATF2 meeting LAPP; David Urner 13 Vertical table for mounting interferometer (made of non-magnetic SUS honeycomb core) Beam Horizontal table for mounting vertical table ( made of steel honeycomb core) Cover for preventing LASAR (Base plate for Ensure flatness) Table for F.F.magnets Horizontal position adjustment Rigid mount for optical table -top view outline

14. 24.09.07 ATF2 meeting LAPP; David Urner 14 CSM mount at magnet end Survey holes What is size of cutouts required to mount survey nests CSM mounted on this platform Observe motion of pole tips with respect to platform on upstream end of magnet

15. 24.09.07 ATF2 meeting LAPP; David Urner 15 CSM mount at Shintake monitor end Shintake monitor table Shintake monitor vacuum vessel IP BPM Beam line CSM vacuum chamber Position monitor to measure IP-BPM position with respect to platform Platform used to mount CSM

16. 24.09.07 ATF2 meeting LAPP; David Urner 16 Next steps Develop mounting structure compatible with ATF2 layout Is there space for a cross brace between Shintake monitor and magnet table Can we attach our system to magnet table Develop real designs for platforms on magnet and Shintake monitor side. Make conceptual design for CSM vacuum vessel.

17. 24.09.07 ATF2 meeting LAPP; David Urner 17 Plans Develop CSM Monitor ATF2 IP Laser frequency stabilisation with 87 Rb standard Required for stable FFI Demonstrate nm resolution in vacuo Install interferometers into vacuum drum Continue analysis software collaboration with LiCAS Analysis framework Adapt LiCAS readout hardware / software

18. 24.09.07 ATF2 meeting LAPP; David Urner 18 Simplified Schematic: Frequency stabilisation Frequency standard: 87 Rb D 2 line at 780 nm

19. 24.09.07 ATF2 meeting LAPP; David Urner 19 Frequency standard : 87 Rb D 2 line at 780 nm Take ultra – narrow line-width laser at 1560 nm Amplify with EDFA (erbium doped fibre) Frequency double in PPLN to produce 780 nm Use saturated absorption spectroscopy 87 Rb to pick out hyperfine structure Lock source laser to peak providing stability of a few kHz (compared to 1 MHz without Rb) At 10 m range, 1 MHz limits resolution to 5 nm locked laser (theoretically 20 pm) other errors will take over