1. G. Trad on the behalf of the BSRT team Emittance meeting 04/11/2015

2. 2 G. Trad- BSRT status- Emittance Meeting  Introduction  Heating of the extraction system  BSRT optical systems  Calibration techniques  Results  BSRT in operation  Miscellaneous  Conclusions and Outlook

3. 3 G. Trad- BSRT status- Emittance Meeting Bunch Length Evolution : 1.3 ns -> 0.8 ns 2000+ bunches Total intensity: 2.3.e14 =>Maximum Temperature excursion 3 o C Fill 4538 (24.4 h SB) ~ 3 o C

4. 4 G. Trad- BSRT status- Emittance Meeting BSRT optics consist in 2 stages imaging system B1 & B2 At injection 2 Lenses optimized for imaging at λ=500 -> 600 nm (L1: φ=76 mm, f~4800 mm ; L2: φ=25 mm, f~300 mm ) Source Undulator SR light is available only in the aforementioned range B1 Additional system used for interferometry R&D, optimized for λ=550 nm (L1: φ=100 mm, f~816 mm ; L2: φ=25 mm, f~18 mm ) In absence of slits, this could be used as an imaging line featuring new optical properties (f#...) At FlatTop 2 Lenses optimized for imaging at λ=250 nm (L1: φ=76 mm, f~4800 mm ; L2: φ=25 mm, f~300 mm ) Source D3 dipole SR light is broadband, the choice of the lower wavelength in the visible range (NUV) aims to reduce the effect of diffraction

5. 5 G. Trad- BSRT status- Emittance Meeting By design, BSRT measurement should be calibrated w.r.t. WS => BSRT emittance measurements accuracy is dictated by WS precision and accuracy SR imaging technique: SR Optical System (Magnification, resolution) Optical System (Magnification, resolution) Detector Profile on Camera -> Gaussian Fit -> σ meas in the image plane -> Normalizing by the optical system magnification -> σ meas in the object plane -> Correcting by the optical resolution -> σ BSRT at the SR source location -> Using the machine optics parameter -> Emittance calculation

6. 6 G. Trad- BSRT status- Emittance Meeting MODE A: Calibration using BPM & WS data Bumps in IR 4 + BPM data Obtained from WS meas. Magnification SR image centroid shift on the camera is proportional to the SR source displacement (beam orbit bumps). We apply local Bumps around IR4, the BPMs are used to calculate the beam displacement (4 BPMs around IR4 are used) N.B: For every optical system configuration (lens position focusing on a different point in the source plane) this exercise should be repeated. LSF Once the beam size in the object (SR source) plane is obtained, A correction factor is applied to the BSRT measurement such as the inferred emittance is the same at both instruments.

7. 7 G. Trad- BSRT status- Emittance Meeting MODE A: Calibration using BPM & WS data

8. 8 G. Trad- BSRT status- Emittance Meeting MODE B: Calibration based only on WS data % ---> MAGNIFICATION = sqrt(betaRatio/slope); % ---> LSF = sqrt(intercept*slope/betaRatio); Y slope X intercept Deconvolution assuming Gaussian beam profile and Gaussian LSF

9. 9 G. Trad- BSRT status- Emittance Meeting MODE B: Calibration based only on WS data

10. 10 G. Trad- BSRT status- Emittance Meeting CALIBRATION Based on WSCALIBRATION Based on BPM B1 Hor B1 Ver B2 Hor B2 Ver MAG : 68.8 µm/px LSF : 315.4 µm MAG : 76.4 µm/px LSF : 228 µm MAG : 65.4 µm/px LSF : 345 µm MAG : 70 µm/px LSF : 283 µm MAG : 77.4 µm/px LSF : 370 µm MAG : 83.5 µm/px LSF : 310 µm MAG : 67.4 µm/px LSF : 370 µm MAG : 74.8 µm/px LSF : 390 µm *1.068 *1.03 *1.092 *1.125 Significant difference reaching even 12% in some cases BSRT scale from BPM is always greater then when calculated from WS Error could originate from BPM scaling factors WS scaling conversion factors from ADC steps to mm.

11. G. Trad- BSRT status- Emittance Meeting Using WS data for magnification 11

12. 12 G. Trad- BSRT status- Emittance Meeting Using BPM data for magnification

13. 13 G. Trad- BSRT status- Emittance Meeting  BSRT is reliably operational in 2015 Has been crucial for beam-beam, instabilities and EC studies Crosschecked with independent measurement (op scans)  Several challenges in Run II, mainly the increasing number of bunches (limited time at injection and limited acquisition speed) Detector lifetime (clear dependence of the beam size on the spot position)  The Server is continuously being upgraded by Enrico to optimize the system (priority scanning for freshly injected beams, Off-centring the beam spot, Compensating eventual camera loss of sensitivity, investigating effects of non Gaussian resolution)  Logging of beam profile on request is available (LOW dynamic range, interpretation very challenging especially at FT)

14. 14 G. Trad- BSRT status- Emittance Meeting  Comparing BSRT optical system vs BSRI optical system (in imaging) N.B: BSRI system could be further optimized finding an optimum focusing point. However it requests additional calibration time Vertical Spread reflects the instrument precision

15. 15 G. Trad- BSRT status- Emittance Meeting  Comparing BSRT optical system vs BSRI optical system (in imaging) N.B: BSRI system could be further optimized finding an optimum focusing point. However it requests additional calibration time BSRT BSRI H MAG:68.8 µm/px 10.9 µm/px LSF: 315.4 µm 348 µm V MAG:76.4 µm/px 10.7 µm/px LSF: 228 µm 293 µm This week an MD will be carried out to compare the performance of the NUV vs visible BSRT imaging systems. This will allow investigating the benefits of an optical system with shorter focal lengths

16. 16 G. Trad- BSRT status- Emittance Meeting  Vertical beam size measurement by interferometry Bunch 0 Bunch 1785 Data acquired at the end calibration studies (F-4513), with a small emittance bunch (0) and a blown up bunch (1785) Slit scan from D=3mm to D=21 mm

17. 17 G. Trad- BSRT status- Emittance Meeting  Vertical beam size measurement by interferometry σ = 185/200 µm Instead of σ = 320/450 µm !!!

18. 18 G. Trad- BSRT status- Emittance Meeting  BSRT is operational and very well calibrated to WS  Investigations still take place for improving the cross calibration by reducing the uncertainties on WS measurements (noise studies).  Profit from MDs parasitically for interferometry system calibration.  New acquisition card will be deployed during winter shutdown that will fasten the acquisitions to a max of 50 fps, reducing the total time of beam scan.  For BSRT consolidation new digital cameras will be installed to further fasten the acquisition to some 100s fps. New intensifiers will also be installed featuring higher sensitivity, better profile and higher SNR (~summer 2016).  A beam halo monitoring system will be installed in B2 during winter shutdown.