1 / 21

High Dynamic Range Beam Imaging with a Digital Optical Mask*

High Dynamic Range Beam Imaging with a Digital Optical Mask*. Presented by Tim Koeth (UMD) on behalf of R.B. Fiorito, H.D. Zhang, A. Shkvarunets UMD, College Park, Maryland S. Zhang, S. V. Benson, D. Douglas, F. G. Wilson JLAB, Newport News, Virginia.

Download Presentation

High Dynamic Range Beam Imaging with a Digital Optical Mask*

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. High Dynamic Range Beam Imaging with a Digital Optical Mask* Presented by Tim Koeth (UMD) on behalf of R.B. Fiorito, H.D. Zhang, A. Shkvarunets UMD, College Park, Maryland S. Zhang, S. V. Benson, D. Douglas, F. G. Wilson JLAB, Newport News, Virginia DITANET Beam Diagnostics Conference November 9-11, 2011, Seville, Spain *Work Funded by US ONR, DOD JTO and DOE Office of HEP

  2. Outline • Introduction • Motivation and Challenges of Halo Measurements • Current diagnostic techniques • New Adaptive Halo Imaging Technique usingDigital Micromirror Device (DMD) • Experimental Results • University of Maryland Electron Ring (UMER) • JLAB FEL • Future Plans

  3. Motivation and Challenges Negative effects of Beam Halo • Beam Loss • Activation of Beam line components • Emittance Growth • Emission of Secondary Electrons • Increased Noise in Detectors • Challenges to diagnostics of halos • Need high dynamic range: >~105 • Adaptive to variable beam core

  4. Previous Experimental Methods Wire Scanner and Scraper Assembly Low-Energy Demonstration Accelerator - LANL DR: 105 Ionization beam profile monitor DR: 103 Passive Spatial Filtering solar coronagraphy applied to beams DR: 106-107 P. Cameron, et al. Proc. of PAC99: 2114-2116, 1999 Imaging Techniques T. Mitsuhashi, EPAC 2004. T.P.Wangler, et. al., Proc. PAC01 High Dynamic Range Camera Spectra-Cam CID $$ DR >105 measured with laser C.P. Welsch, et. , Proc. SPIE 6616,9 (2007).

  5. 120 Digital Micro-mirror Device* *DLPTM TexasInstruments Inc. Array dimensions: 14 x 10 mm Pixels: 1024 x 768, Pixel dimension: 14x14 mm Switching rate: 9600 fps Individual pixel addressable Used in HD TV & Projectors Available as development ‘kits’ Optimized to visible, IR, UV

  6. Beam Halo Imaging System using DMD developed at UMD* *R.Fiorito, H.Zhang, A. Shkvarunets, et. al. Proc. BIW2010 Pixels near saturation Beam optical radiation Source Source Mirror Mirror L1 L1 Computer 32 mm Computer L2 L2 L3 32 mm L3 L4 L4 Halo Light Core Light Image 2 900 Frames 180 Frames Camera Sensor Camera Sensor Mask Image 1 DMD DMD Pixels near saturation DR >105 Two compensations are needed, DMD rotated 45o & path length

  7. Scheimpflug compensation Lens Scheimpflug intersection 12 0 24 0 Target reflected light θ φ Micro-mirrors Incident light Image on DMD DMD u v mirror Lens focus length f Image on CCD Image on DMD

  8. DMD Imaging Experiments on University of Maryland Electron Ring (UMER) Screen Screen

  9. Dynamic Range measurement of imaging system Phosphor screen image of 21 mA beam 32mm 20 275 1000 Integration Frames: 290 pixel 2000 3000 5000

  10. 0 - 1 Log I/I0 - 2 - 3 - 4 - 5 Dynamic Range Measurement at UMER 32mm 32 mm

  11. Spatial Filtering Ability of DMD Beam on, DMD all on Beam on, DMD all off 32mm 180 180 21 mA beam

  12. Comparison of Images obtained with DMD and Mirror DMD all on (with Scheimplug compensation) Simple Mirror (no compensation) DMD all floating (no compensation)

  13. Quadrupole Screen Quadrupole Induced Halo Experiments on UMER Screen

  14. Demonstration of adaptive threshold masking Quadrupole Current IQ 82.9%IQ 66.3%IQ 49.7%IQ 32mm (a) y x 70 45 45 60 (b) 640 660 250 280

  15. Non Interceptive Beam/Halo Imaging at JLAB using Optical Synchrotron Radiation Bending Magnet Quadrupoles

  16. Quadrupole Scan Using OSR with Tune-up Beam (E=135 MeV, I= 0.32mA: 2Hz rep-rate, 250ms macro, 4.68MHz micro, 135pC/micro ) 4 mm 0 G 500 G -500 G 300 G 0G Quad strength -700 G -1000 G -1700 G -2000 G -2500 G -3000 G

  17. OSR Halo Imaging of JLAB CW beam with DMD threshold mask (I = 0.63 mA, 4.68MHz, 65pc/micropulse, l= 654nm x 90nm , ND=0.4 ) 11.6 mm 0.04 s 0.18 s 11.6 mm 1.6 s 42 s 6.5 s

  18. Measurement of Dynamic Range of imaging system

  19. Measurement of Dynamic Range of 0.6 mA CW Beam

  20. Reconstructed intensity distribution J(x,y) and calculated total radiant energy ETotal (1- 10-6 ) Jmax (1 -10-2 ) Jmax (10-2 -10-6) Jmax

  21. Summary • Results • Developed and tested high-dynamic range ( DR ~105 ) halo diagnostic imaging system using a phosphor screen + DMD at UMER • Developed a non interceptive OSR DMD imaging system to observe beam halo at JLAB FEL under CW operating conditions; with measured DR > 106 . • Performed quad scan of JLAB tune-up beam using OSR • Future plans • UMER: Do time-resolved halo imaging and multi-turn halo evolution studies at UMER using DMD to study/mitigate factors effecting halo • JLAB: • Short terms: Verify and possibly improve DR >~10(5) of present system • 1a) Improve background measurements and verify halo is not due to stray light from upstream internal sources • 1b) decrease optical magnification onto DMD and /or increase current density via current, focusing/tune; • Long term: Extend DR of halo measurement to limit: • 1) add Lyot and/or apodizing stops to decrease effect of diffraction • 2) improve optical transport with enclosures and antireflection coating on optics port to further reduce any external stray light • Compare emittance measurements using OTR and OSR quad scans • Explore possibility of using DMD to measure halo/core emittances and to do optical phase space mapping (optical analogy of pepper pot technique)

More Related