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Undulator Radiation & FEL
U.S. Particle Accelerator School January 25 – February 19, 2021 VUV and X-ray Free-Electron Lasers Introduction, Electron Motions in an Undulator, Undulator Radiation & FEL Dinh C. Nguyen,1 Petr Anisimov,2 Nicole Neveu1 1 SLAC National Accelerator Laboratory 2 Los Alamos National Laboratory LA-UR-21-20610 Monday (Jan 25) Lecture Outline Time • VUV and X-ray FELs in the World 10:00 – 10:30 • Properties of electromagnetic radiation 10:30 – 10:50 • Break 10:50 – 11:00 • Electron motions in an undulator 11:00 – 11:20 • Undulator radiation 11:20 – 11:40 • Introduction to FELs 11:40 – Noon 2 VUV and X-ray FELs in the World 3 World Map of VUV and X-ray FELs FLASH FERMI European XFEL Italy Germany SPARC LCLS Italy SwissFEL POLFEL LCLS-II & LCLS-II-HE Switzerland Poland USA PAL XFEL S. Korea SACLA Japan SDUV-SXFEL SHINE China Blue=VUV to Soft X-ray 4 Purple=Soft to Hard X-ray Sub-systems of an RF Linac Driven X-ray FEL An RF-linac driven XFEL has the following sub-systems in order to produce Low-emittance • PHOTOINJECTOR to generate low-emittance electrons in ps bunches electron beams • RF LINAC to accelerate the electron beams to GeV energy • BUNCH COMPRESSORS to shorten the bunches and produce kA current High peak current • LASER HEATER to reduce the microbunching instabilities • BEAM OPTICS to transport the electron beams to the undulators • UNDULATORS to generate and amplify the radiation in a single pass Single-pass, high- gain X-ray FEL • DIAGNOSTICS to characterize the electron & FEL beams Laser Photoinjector heater L2 BC2 L1 L3 Optics -
Status and Vision for Structural Biology at the Canadian Light Source P
Vol. 121 (2012) ACTA PHYSICA POLONICA A No. 4 Proceedings of the 9th National Symposium of Synchrotron Radiation Users, Warsaw, September 2627, 2011 Status and Vision for Structural Biology at the Canadian Light Source P. Grochulskia;b∗, M.N. Fodjea;c and G. Georged a Canadian Light Source, 101 Perimeter Road, Saskatoon, SK S7N 0X4 Canada b College of Pharmacy and Nutrition, University of Saskatchewan, 110 Science Place, Saskatoon, SK S7N 5C8, Canada c Department of Biochemistry, University of Saskatchewan, 107 Wiggins Road, Saskatoon SK S7N 5E5, Canada dDepartment of Geology, University of Saskatchewan, 114 Science Place, Saskatoon, SK S7N 5E2, Canada The status and vision for Structural Biology at the Canadian Light Source (CLS) is presented. The beamlines that have been described in the paper represent a Canadian national resource that is available to science and industry world-wide. They include state-of-the-art infrastructure and include specialized capabilities, many of which are not available elsewhere, including macromolecular crystallography, biological X-ray spec- troscopy, soft X-ray spectromicroscopy, as well as small angle and wide angle X-ray scattering beamlines. The vision for Structural Biology at the Canadian Light Source is signicantly enhanced by the synergies and col- laborations between the users of the dierent beamlines and by the strengths of the scientic personnel and trainees. PACS: 87.64.kd, 87.80.Dj 1. Introduction TABLE I 2.53.0 GeV synchrotron facilities worldwide and the The Canadian Light Source (CLS) is a 2.9 GeV na- number of MX, BioXAS and BioSAXS/WAXS beamlines tional synchrotron radiation facility located at the Uni- versity of Saskatchewan in Saskatoon. -
FEL Physics Summary
VUV and X-Ray Free Electron Lasers: The Technology and Its Scientific Promise William Barletta and Carlo Rizzuto Sections I & III – Motivations & FEL Physics List of symbols fine structure constant dimensionless vector potential aw horizontal Twiss x bunching parameter b mean resolution error of BPMs BPMres position error of BPMs BPMpos remanent field BR undulator magnetic field strength Bw horizontal Twiss x speed of light c mean phase error in undulator penetration depth δp horizontal dispersion Dx derivative of Dx D´x FEL beam diameter on optic Dw energy chirp from CSR E/E beam emittance electron charge e beam energy E peak electric field in gun Eo normalized emittance n energy in the FEL pulse EPulse longitudinal space charge force Fsc angle of incidence j i 1 2 relativistic factor (E/ me c ) optical function in transport H magnetic coercivity HC Alfven current at =1 IAo beam current Ib BBU threshold current IBBU undulator parameter K mean undulator strength Krms undulator spatial frequency kw gain length LG th m harmonic wavelength m plasma wavelength P radiation wavelength r undulator wavelength w root of gain equation harmonic number m electron mass me number of electrons Ne electron density ne number of undulator periods Nu radiation power P input laser power Plaser noise power Pn pole roll angle error BNP (or Pierce) parameter quantum FEL parameter ´ atom density A quality factor Q dipole quality factor Qdipole FEL energy constraint ratio r1 FEL emittance constraint ratio r2 FEL diffraction constraint ratio r3 classical radius of electron re bend angle in undulator bend angle in achromat 2 th phase of i electron i kick relative to each pole error j mean energy spread of electrons e bunch length z relativistic plasma frequency p distance along undulator z mean longitudinal velocity <vz> impedance of free space Zo Rayleigh range ZR 3 I. -
Insertion Devices Lecture 4 Undulator Magnet Designs
Insertion Devices Lecture 4 Undulator Magnet Designs Jim Clarke ASTeC Daresbury Laboratory Hybrid Insertion Devices – Inclusion of Iron Simple hybrid example Top Array e- Bottom Array 2 Lines of Magnetic Flux Including a non-linear material like iron means that simple analytical formulae can no longer be derived – linear superposition no longer works! Accurate predictions for particular designs can only be made using special magnetostatic software in either 2D (fast) or 3D (slow) e- 3 Field Levels for Hybrid and PPM Insertion Devices Assuming Br = 1.1T and gap of 20 mm When g/u is small the impact of the iron is very significant 4 Introduction We now have an understanding for how we can use Permanent Magnets to create the sinusoidal fields required by Insertion Devices Next we will look at creating more complex field shapes, such as those required for variable polarisation Later we will look at other technical issues such as the challenge of in-vacuum undulators, dealing with the large magnetic forces involved, correcting field errors, and also how and why we might cool undulators to ~150K Finally, electromagnetic alternatives will be considered 5 Helical (or Elliptical) Undulators for Variable Polarisation We need to include a finite horizontal field of the same period so the electron takes an elliptical path when it is viewed head on We want two orthogonal fields of equal period but of different amplitude and phase 3 independent variables Three independent variables are required for the arbitrary selection of any polarisation state -
2006Spring.Pdf
− X8 PROTEUM THE ULTIMATE STRUCTURAL BIOLOGY SYSTEM When you need the best system for Structural Biology, the Bruker X8 PROTEUM offers high-throughput screening AND superb high resolution data in one uncompromising package. With our MICROSTAR family of generators, you can rely on the extremely intense micro-focus X-ray beam coupled with the ultra-bright HELIOS optics to handle everything from small crystals to large unit cells With over 700135 detector CCD detectors for speed, installed, sensitivity, we know size and how dynamic to optimize range the to give PLATINUM you the best data possible in the home lab Our KAPPA goniometer’s high precision mechanics allow you to orient the sample along any axis in reciprocal space, while having easy access to mount, cool or anneal your crystals Get the best data, get the fastest system, get the power to solve your structures – X8 PROTEUM. BRUKER ADVANCED X-RAY SOLUTIONS North America: BRUKER AXS INC Tel. (+1) (608) 276-3000 Fax (+1) (608) 276-3006 www.bruker-axs.com [email protected] Germany: BRUKER AXS GMBH Tel. (+49) (721) 595- 2888 Fax (+49) (721) 595-4587 www.bruker-axs.de [email protected] Netherlands: BRUKER AXS BV Tel. (+31) (15) 215-2400 Fax (+31) (15) 215-2500 www.bruker-axs.nl [email protected] American Crystallographic Association * REFLECTIONS *see page 9 for notes on our new name and for new logo possibilities Cover: Images from Warren Award Recipient Charles Majkrazk and his colleagues; see page 25. ACA HOME PAGE: hwi.buffalo.edu/ACA/ Table of Contents 3 President’s -
Beam Dynamics of the Superconducting Wiggler on the Ssrf Storage Ring
Submitted to ‘Chinese Physics C’ BEAM DYNAMICS OF THE SUPERCONDUCTING WIGGLER ON THE SSRF STORAGE RING * ZHANG Qing-Lei(张庆磊)1,2 TIAN Shun-Qiang(田顺强)1 JIANG Bo-Cheng(姜伯承)1 XU Jie-Ping(许皆平) 1 ZHAO Zhen-Tang(赵振堂)1;1) 1 Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, P.R. China 2 University of Chinese Academy of Sciences, Beijing 100049, P.R. China * Supported by National Natural Science Foundation of China (11105214) 1) E-mail: [email protected] Abstract In the SSRF Phase-II beamline project, a Superconducting Wiggler (SW) will be installed in the electron storage ring. It may greatly impact on the beam dynamics due to the very high magnetic field. The emittance growth becomes a main problem, even after a well correction of the beam optics. A local achromatic lattice is studied, in order to combat the emittance growth and keep the good performance of the SSRF storage ring, as well as possible. Other effects of the SW are simulated and optimized as well, including the beta beating, the tune shift, the dynamic aperture, and the field error effects. Key word SSRF storage ring, superconducting wiggler, beam dynamics, Accelerator Toolbox PACS 29.20.db, 41.85.-p INTRODUCTION Shanghai Synchrotron Radiation Facility (SSRF) is a third generation light source with the beam energy of 3.5GeV [1-3]. It has been operated for users’ experiments since 2009. There are 20 straight sections in the storage ring of SSRF, including 4 long straight sections (LSSs) and 16 standard straight sections (SSSs). -
Synchrotron Light Source
Synchrotron Light Source The evolution of light sources echoes the progress of civilization in technology, and carries with it mankind's hopes to make life's dreams come true. The synchrotron light source is one of the most influential light sources in scientific research in our times. Bright light generated by ultra-rapidly orbiting electrons leads human beings to explore the microscopic world. Located in Hsinchu Science Park, the NSRRC operates a high-performance synchrotron, providing X-rays of great brightness that is unattainable in conventional laboratories and that draws NSRRC users from academic and technological communities worldwide. Each year, scientists and students have been paying over ten thousand visits to the NSRRC to perform experiments day and night in various scientific fields, using cutting-edge technologies and apparatus. These endeavors aim to explore the vast universe, scrutinize the complicated structures of life, discover novel nanomaterials, create a sustainable environment of green energy, unveil living things in the distant past, and deliver better and richer material and spiritual lives to mankind. Synchrotron Light Source Light, also known as electromagnetic waves, has always been an important means for humans to observe and study the natural world. The electromagnetic spectrum includes not only visible light, which can be seen with a naked human eye, but also radiowaves, microwaves, infrared light, ultraviolet light, X-rays, and gamma rays, classified according to their wave lengths. Light of Trajectory of the electron beam varied kind, based on its varied energetic characteristics, plays varied roles in the daily lives of human beings. The synchrotron light source, accidentally discovered at the synchrotron accelerator of General Electric Company in the U.S. -
Insertion Devices Lecture 1 Introduction to Synchrotron Radiation
Insertion Devices Lecture 1 Introduction to Synchrotron Radiation Jim Clarke ASTeC Daresbury Laboratory Program 4th Feb 10.30 Introduction to SR 4th Feb 11.45 Wigglers and Undulators 11th Feb 10.30 Undulator Radiation and Realisation 11th Feb 11.45 Undulator Magnet Designs 11th Feb 14.00 Tutorial Please interrupt and ask questions during the lectures !!! 2 Course Book The vast majority of the material presented is from my book, you will find much more detail in there, derivations of all the equations, and also other supplementary information. The Science and Technology of Undulators and Wigglers, J. A. Clarke, Oxford University Press, 2004 (Oxford series on Synchrotron Radiation - 4) It is available in the Daresbury Library 3 Why is Synchrotron Radiation so Important? All accelerator scientists and engineers need to understand SR as it impacts directly on many areas of accelerator design and performance o RF o Diagnostics o Vacuum design o Magnets o Beam Dynamics o It affects all charged particles o Light sources and Free Electron Lasers are a major “customer” of advanced accelerators All processes which change the energy of particles are important – SR is one of the most important processes 4 Introduction to Synchrotron Radiation Synchrotron Radiation (SR) is a relativistic effect Many features can be understood in terms of two basic processes: Lorentz contraction and Doppler shift Imagine that a relativistic charged particle is travelling through a periodic magnetic field (an undulator) In the particles rest frame it sees a magnetic -
Triple Period Undulator
10th Int. Partile Accelerator Conf. IPAC2019, Melbourne, Australia JACoW Publishing ISBN: 978-3-95450-208-0 doi:10.18429/JACoW-IPAC2019-TUPRB022 TRIPLE PERIOD UNDULATOR A. Meseck ∗ 1 , J. Bahrdt, W. Frentrup, M. Huck, C. Kuhn, C. Rethfeldt, M. Scheer and E. Rial, Helmholtz Zentrum Berlin, Berlin, Germany, 1also at Johannes Gutenberg University Mainz, Germany Abstract Very recently, a 17 mm period CPMU with a 5.5 mm min- imum operational gap (CPMU17) was installed in BESSY Insertion devices are one of the key components of mod- II ring [1]. It was designed and built by HZB as a part of the ern synchrotron radiation facilities. They allow for genera- canted double undulator system for the new Energy Mate- tion of radiation with superior properties enabling experi- rials in-situ Laboratory (EMIL) at BESSY II [2]. EMIL is ments in a variety of disciplines, such as chemistry, biology, also served by a 48 mm period APPLEII undulator (UE48), crystallography and physics to name a few. For future cut- built at HZB. The double undulator system covers an energy ting edge experiments in soft and tender x-rays users require range from 60 eV to 6000 eV. high flux and variable polarization over a wide photon energy range independent of other desired properties like variable UE48 provides radiation with variable polarization, pulse length, variable timing or Fourier transform limited whereas the CPMU17 delivers radiation with a fixed polar- pulses. In this paper, we propose a novel ID-structure, called ization like the other already-existing in-vacuum cryogenic Triple Period Undulator (TPU), which allows us to deliver a undulators. -
X-Ray Photoelectron Spectroscopy of Hydrogen and Helium 12 February 2019
X-ray photoelectron spectroscopy of hydrogen and helium 12 February 2019 This work demonstrated that ambient pressure X- ray photoelectron spectra of hydrogen and helium can be obtained when a bright-enough X-ray source is used, such as at the National Synchrotron Light Source II. In the case of helium gas, the spectrum shows a symmetric peak from its only orbital. In the case of hydrogen gas molecules, an asymmetric peak is observed, which is related to the different possible vibrational modes of the final state. The hydrogen X-ray beam induces photo-ejection of an electron from 2 (left) hydrogen and (right) helium . Credit: US molecule vibrational structure is evident in the H 1s Department of Energy spectrum. More information: Jian-Qiang Zhong et al. Synchrotron-based ambient pressure X-ray For the first time scientists measured the photoelectron spectroscopy of hydrogen and vibrational structure of hydrogen and helium atoms helium, Applied Physics Letters (2018). DOI: by X-rays. The results disprove the misconception 10.1063/1.5022479 that it's impossible to obtain X-ray photoelectron spectroscopy (XPS) spectra of hydrogen and helium, the two lightest elements of the Periodic Table. This was thought to be the case due to low Provided by US Department of Energy probabilities of electron ejection from these elements induced by X-rays. Unparalleled beam brightness at the National Synchrotron Light Source-II significantly increases the probability of a photon colliding with a gas atom at ambient pressures. The beamline makes it possible to use XPS to directly study the two most abundant elements in the universe. -
A Superconducting 7T Multipole Wiggler for the Bessy Ii Synchrotron Radiation Source*
Proceedings of the 2001 Particle Accelerator Conference, Chicago A SUPERCONDUCTING 7T MULTIPOLE WIGGLER FOR THE BESSY II SYNCHROTRON RADIATION SOURCE* D. Berger4,M.Fedurin2, M. Mezentsev2,S.Mhaskar3, V. Shkaruba2, F. Schaefers1, M. Scheer1, E. Weihreter1 1 BESSY, Einsteinstraße 15, 12489 Berlin, Germany, 2 BINP, Acad. Lavrentiev prospect 11, 630090 Novosibirsk, Russia, 3 CAT, Indore 452 013, Madhya Pradesh, India, 4 Hahn-Meitner-Institut, Glienicker Straße 100, 14109 Berlin, Germany Abstract Table 1: Multipol wiggler design parameters To generate hard X-ray beams for residual stress critical energy @ 1,9 GeV 16.8 keV analysis and for magnetic scattering using the BESSY II ring, a 7T wiggler with 17 poles is under development. max. field on axis 7.0 T The wiggler is designed for a critical energy of 16.8 keV max.fieldoncoils 8.1T with a 13 mm vertical free aperture and an inner chamber periode length 148 mm on a temperature of 20 K. Essential aspects of the number of poles 17 conceptual magnet layout are discussed, e.g. coil and horiz. beam aperture 110 mm yoke geometry, and vacuum chamber design. A prototype vert. beam aperture 13 mm structure with 7 poles has already been built to verify the magnetic (iron) gap 19 mm technical layout of the wiggler. First experimental results stored magnetic energy 450 kJ for the prototype magnet are presented, demonstrating total radiation power (1.9 GeV, 500 mA) 56 kW that a maximum field of 7.3 T can be obtained with the present design. strength has been chosen. Therefore the beam orbit 1 INTRODUCTION oscillates horizontally around the vertical symmetry plane The BESSY II storage ring is operating as a high of the magnet with the advantage that most of the brilliance Synchrotron radiation (SR) source for the VUV influence of the integral sextupole term on the beam will and soft X-ray spectral range. -
Integumentary Structure and Composition in an Exceptionally Well-Preserved Hadrosaur (Dinosauria: Ornithischia)
Integumentary structure and composition in an exceptionally well-preserved hadrosaur (Dinosauria: Ornithischia) Mauricio Barbi1,*, Phil R. Bell2,*, Federico Fanti3,4, James J. Dynes5, Anezka Kolaceke1, Josef Buttigieg6, Ian M. Coulson7 and Philip J. Currie8 1 Department of Physics, University of Regina, Regina, Saskatchewan, Canada 2 School of Environmental and Rural Science, University of New England, Armidale, New South Wales, Australia 3 Dipartimento di Scienze Biologiche, Geologiche e Ambientali, Alma Mater Studiorum, Università di Bologna, Bologna, Italy 4 Museo Geologico Giovanni Capellini, Università di Bologna, Bologna, Italy 5 Canadian Light Source Inc., University of Saskatchewan, Saskatoon, Saskatchewan, Canada 6 Department of Biology, University of Regina, Regina, Saskatchewan, Canada 7 Department of Geology, University of Regina, Regina, Saskatchewan, Canada 8 Biological Sciences, University of Alberta, Edmonton, Alberta, Canada * These authors contributed equally to this work. ABSTRACT Preserved labile tissues (e.g., skin, muscle) in the fossil record of terrestrial vertebrates are increasingly becoming recognized as an important source of biological and tapho- nomic information. Here, we combine a variety of synchrotron radiation techniques with scanning electron and optical microscopy to elucidate the structure of 72 million- year-old squamous (scaly) skin from a hadrosaurid dinosaur from the Late Cretaceous of Alberta, Canada. Scanning electron and optical microscopy independently reveal that the three-dimensionally preserved scales are associated with a band of carbon-rich layers up to a total thickness of ∼75 microns, which is topographically and morphologically congruent with the stratum corneum in modern reptiles. Compositionally, this band deviates from that of the surrounding sedimentary matrix; Fourier-transform infrared spectroscopy and soft X-ray spectromicroscopy analyses indicate that carbon appears Submitted 27 April 2019 predominantly as carbonyl in the skin.