SLAC National Accelerator Center

Slides:



Advertisements
Similar presentations
Optics and Photonics Selim Jochim together with Dr. K. Simeonidis
Advertisements

Optics and Photonics Selim Jochim MPI für Kernphysik und Uni Heidelberg Website for this lecture:
FINESSE FINESSE Frequency Domain Interferometer Simulation Versatile simulation software for user-defined interferometer topologies. Fast, easy to use.
Design and Experimental Considerations for Multi-stage Laser Driven Particle Accelerator at 1μm Driving Wavelength Y.Y. Lin( 林元堯), A.C. Chiang (蔣安忠), Y.C.
Lab 1 Paraxial Optics Lab in 106A. Look at paraxial optics rules Use a bi-convex singlet at 1:1 conjugates Do it double pass so can see image Lateral.
Chapter 2 Propagation of Laser Beams
Ray matrices The Gaussian beam Complex q and its propagation Ray-pulse “Kosten- bauder” matrices The prism pulse compressor Gaussian beam in space and.
 Light can take the form of beams that comes as close
VARISPOT FS BEHAVIOR IN COLLIMATED AND DIVERGING BEAMS: THEORY AND EXPERIMENTS Liviu Neagu, Laser Department, NILPRP, Bucharest-Magurele, Romania.
Adnan Doyuran a, Joel England a, Chan Joshi b, Pietro Musumeci a, James Rosenzweig a, Sergei Tochitsky b, Gil Travish a, Oliver Williams a a UCLA/Particle.
Course outline Maxwell Eqs., EM waves, wave-packets
Gaussian Beam Propagation Code
Foundations of Physics
1 ILC Bunch compressor Damping ring ILC Summer School August Eun-San Kim KNU.
Chapter 31 Images.
Chapter 26 Geometrical Optics. Units of Chapter 26 The Reflection of Light Forming Images with a Plane Mirror Spherical Mirrors Ray Tracing and the Mirror.
FLAO Alignment Procedures G. Brusa, S. Esposito FLAO system external review, Florence, 30/31 March 2009.
Aperture Pupil (stop) Exit Pupil Entrance Pupil.
Geometric Optics of thick lenses and Matrix methods

First THz Measurements at FACET Ziran Wu, Alan Fisher, Henrik Loos FACET 2011 Users Meeting
Properties of Multilayer Optics An Investigation of Methods of Polarization Analysis for the ICS Experiment at UCLA 8/4/04 Oliver Williams.
Copyright © 2009 Pearson Education, Inc. Chapter 32 Light: Reflection and Refraction.
Overview of Proposed Parameter Changes Linac Coherent Light Source Stanford Synchrotron Radiation Laboratory Stanford Linear Accelerator.
The Ray Vector A light ray can be defined by two co-ordinates: x in,  in x out,  out its position, x its slope,  Optical axis optical ray x  These.
Integration and Alignment of Optical Subsystem Roy W. Esplin Dave McLain.
Chapter 25 Optical Instruments.
Visual Angle How large an object appears, and how much detail we can see on it, depends on the size of the image it makes on the retina. This, in turns,
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 26 Physics, 4 th Edition James S. Walker.
Effective lens aperture Deff
1 Proposal for a Multi-Optical Transition Radiation System in ATF2 A. Faus-Golfe, D. McCormick IFIC – SLAC 11 June th TB/SGC Meeting.
High Harmonic Generation in Gases Muhammed Sayrac Texas A&M University.
Ground Motion + Vibration Transfer Function for Final QD0/SD0 Cryomodule System at ILC Glen White, SLAC ALCPG11, Eugene March 21, 2011.
BROOKHAVEN SCIENCE ASSOCIATES BIW ’ 06 Lepton Beam Emittance Instrumentation Igor Pinayev National Synchrotron Light Source BNL, Upton, NY.
FLAO system test plan in solar tower S. Esposito, G. Brusa, L. Busoni FLAO system external review, Florence, 30/31 March 2009.
Matching recipe and tracking for the final focus T. Asaka †, J. Resta López ‡ and F. Zimmermann † CERN, Geneve / SPring-8, Japan ‡ CERN, Geneve / University.
Fifth ATF2 Project Meeting, dec. 2007, KEK, Japan Emittance measurements with multiple wire-scanners and quadrupole scans in ATF EXT C. Rimbault,
Institute of Atomic and Molecular Sciences, Academia Sinica, Taiwan National Taiwan University, Taiwan National Central University, Taiwan National Chung.
ABSTRACT The design of a complete system level modeling and simulation tool for optical micro-systems is the focus of our research . We use a rigorous.
Resolution Limits for Single-Slits and Circular Apertures  Single source  Two sources.
Fast Electron Temperature Scaling and Conversion Efficiency Measurements using a Bremsstrahlung Spectrometer Brad Westover US-Japan Workshop San Diego,
Grisms Michael Sholl Space Sciences Laboratory 29 March 2003 Practical implementation for SNAP.
Doc.: IEEE /0431r0 Submission April 2009 Alexander Maltsev, Intel CorporationSlide 1 Polarization Model for 60 GHz Date: Authors:
Electromagnetic Waves
Plan in summer shutdown Magnet -SF1FF -Swap of QEA magnet - Multipole field of Final Doublet IP-BSM improvement.
S. Molloy, P. Emma, J. Frisch, R. Iverson, M. Ross, D. McCormick, M. Woods, SLAC, CA, USA S. Walston, Lawrence Livermore National Laboratory, CA, USA V.
14 Sep 2000ASTR103, GMU, Dr. Correll1 ASTR 103--Week 3.
Max Cornacchia, SLAC LCLS Project Overview BESAC, Feb , 2001 LCLS Project Overview What is the LCLS ? Transition from 3 rd generation light sources.
Design options for emittance measurement systems for the CLIC RTML R Apsimon.
New emittance monitor beamline
ATF2 beam operation status Toshiyuki OKUGI, KEK The 9 th TB&SGC meeting KEK, 3-gokan Seminar Hall 2009/ 12/ 16.
Emittance measurements with multiple wire-scanners and quadrupole scans in ATF EXT C. Rimbault, Brossard, P. Bambade (LAL) Main goal : - Try to improve.
GEOMETRICAL OPTICS. Laws of Reflection Laws of Refraction.
06 Oct 05Space Science & Technology Dept1 Solar Orbiter Consortium Meeting 03 Mar 06 Optical Design Of Solar Orbiter Normal Incidence Spectrometer KF Middleton.
SL/BI 16/05/1999DIPAC’99 -- JJ Gras -- CERN SL/BI -- Adaptive Optics for the LEP 2 SR Monitors G. Burtin, R.J. Colchester, G. Ferioli, J.J. Gras, R. Jung,
Spherical Aberration. Rays emanating from an object point that are incident on a spherical mirror or lens at different distances from the optical axis,
Geometrical Optics.
Light and Optics  The Electromagnetic Spectrum  Interference, Diffraction, and Polarization Wave Properties of Light.
G. Trad on the behalf of the BSRT team Emittance meeting 04/11/2015.
Polarization of final electrons/positrons during multiple Compton
SPARCLAB: PW-class Ti:Sa laser+SPARC
Lab 1 Paraxial Optics Lab in 106A.
Electron Beam Diagnostics at REGAE
Accelerator Physics and Engineering Update Jan 6, 2010
Boian Andonov Hristov, Prof. (Ph.D) Bulgarian Academy of Sciences
Optical Design of a Broadband IR Spectrometer
X-Ray Spectrometry Using Cauchois Geometry For Temperature Diagnostics
Accelerator Physics and Engineering Update Jan 6, 2010
Beam size diagnostics using diffraction radiation
Transverse coherence and polarization measurement of 131 nm coherent femtosecond pulses from a seeded FEL J. Schwenke, E. Mansten, F. Lindau, N. Cutic,
Presentation transcript:

SLAC National Accelerator Center Calculations and Simulations of an Infrared Prism Spectrometer for Ultra-Fast Bunch Length Diagnosis at LCLS Julie Cass SULI Program 2011 SLAC National Accelerator Center Advisor Josef Frisch

Overview of Spectrometer Optics 1 90° off-axis parabolic mirrors (OAP) HeNe laser at 632.816 nm (visible) to align optics Alignment complicated when infrared laser is used KRS-5 crystal acts as spectrometer prism, dispersing transition radiation

MATLAB Model: Ray Transfer Matrix Analysis 2 MATLAB Model: Ray Transfer Matrix Analysis MATLAB used to model beam size with ray transfer matrix analysis Ray transfer matrix: 2 x 2 matrices describing each optical element or free space propagated by beam Free space propagation Passage through a lens of focal length f

Gaussian Ray Transfer Matrix Analysis 3 Designed for modeling light rays of negligible waist size HeNe laser is Gaussian - generated a vector to represent the initial beam in terms of a complex beam parameter q R – radius of curvature w – beam width k – normalization constant for second component of beam vector MATLAB code calculates and graphs beam waists

Optical Element Number* 4 Log of Beam Width Optical Element Number* *including free spaces of step size 100um

ZEMAX Simulation 5 Study spectrometer resolution achievable: simulation using optics modeling software ZEMAX ZEMAX offers ray-tracing computations, following paths of perfect geometric rays as they are reflected and refracted Spot size analyzed at two points: (1) Focal point of first OAP (2) Detector surface (focal point of 3rd OAP)

ZEMAX: Adding Mirror Tilts 6 Mirror tilts in increments of 0.05° along optical, horizontal and vertical axes Angles adjusted until beam size similar to measured beam size reached, then compared with estimated misalignment error

ZEMAX: Detector Tilt Dispersion causes chromatic aberrations 7 Dispersion causes chromatic aberrations Detector tilt required New simulation to account for differences in design parameters C. Behrens et al., “Design of a Single-Shot Prism Spectrometer in the Near- and Mid-Infrared Wavelength Range for Ultra-Short Bunch Length Diagnostics”

Results and Analysis

Results: Beam Size at First OAP Focus 8 Measured: 172 um MATLAB: 65 um ZEMAX: Tilts of ~0.4° to change beam size at focus from 0 to 172um Consistent with human error in alignment

Results: Beam Size at Detector Surface 9 Measured: 280 um MATLAB: 38 um Much larger degree of error (~ 7x magnification) ZEMAX: 14 um Tilts of ~1.03° about horizontal/vertical axes needed to achieve measured size Tilts of ~1.07° about optical axis needed to achieve measured size This measurement is much more complicated

Updated Detector Tilt Detector tilt of 45° for optimal focusing 10 Detector tilt of 45° for optimal focusing All wavelengths will not fit on detector surface: range limited by this size rather than KRS-5 transmission 14mm

Conclusions Current alignment leaves significant aberrations 11 Conclusions Current alignment leaves significant aberrations Development of alignment procedures with greater precision Addition of lasers with a range of wavelengths Detector range limited by its size unless: Adjustments are made to current design

Acknowledgements Advisor: Joe Frisch ZEMAX advising : Alan Fischer 12 Acknowledgements Advisor: Joe Frisch ZEMAX advising : Alan Fischer Colleagues: Kiel Williams and Gilles Dongmo-Momo SULI Program Director: Steve Rock DOE and SLAC National Accelerator Laboratory for funding and direction of SULI Program

References [1] Y. Ding et al., “Measurements and Simulations of Ultralow Emittance and Ultrashort Electron Beams in the Linas Coherent Light Source”, PRL 102, 254801, 2009  [2] Linear Coherent Light Source http://lcls.slac.stanford.edu/ [3] K. Williams, “Optical Design of a Broadband Infrared Spectrometer for Bunch Length Measurement at the Linac Coherent Light Source,” SLAC National Accelerator Laboratory SULI Program 2011, Palo Alto, CA  [4] Pyreos Ltd, http://www.pyreos.com/ [5] G. Dongmo-Momo, “Calibration of the Heat Sensor for the Free Electron Laser Bunch Length Measurements,” SLAC National Accelerator Laboratory SULI Program, Palo Alto, CA 2011 [6] MATLAB 7.0.4, The MathWorks Inc. [7] Bahaa E. A. Saleh and Malvin Carl Teich (1991). Fundamentals of Photonics. New York: John Wiley & Sons. Section 1.4, pp. 26-36 [8] Gaussian Beams http://www.rp-photonics.com/ [9] Radiant ZEMAX LLC, http://www.zemax.com [10] C. Behrens et al., “Design of a Single-Shot Prism Spectrometer in the Near- and Mid-Infrared Wavelength Range for Ultra-Short Bunch Length Diagnostics”, DIPAC'11, Hamburg, Germany, 201