Canadian Light Source Starts on 10 December 2003, with ®Rst Beam Being Accumulated ®Ve Days Later
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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. -
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). -
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. -
A New LLRF System for ASTRID and the Proposed ASTRID2
Jørgen S. Nielsen Institute for Storage Ring Facilities (ISA) Aarhus University Denmark ESLS XVIII (25-26/11 2010), Status of the ASTRID2 project 1 ` ASTRID2 is the new synchrotron light source presently being built in Aarhus, Denmark ` Dec 2008: Received 37 MDKr (5 M€) to ◦ Build a new SR light source ◦ Convert ASTRID into a booster ◦ Move existing beam lines x New 2 T Multi Pole Wiggler ` The project should be finished in 2013 ESLS XVIII (25-26/11 2010), Status of the ASTRID2 project 2 ` ASTRID2 main parameters ◦ Electron energy: 580 MeV ◦ Emittance: 12 nm ◦ Beam Current: 200 mA ◦ Circumference: 45.7 m ◦ 6-fold symmetry x lattice: DBA with 12 combined function dipole magnets x Integrated quadrupole gradient ◦ 4 straight sections for insertion devices ◦ Will use ASTRID as booster (full energy injection) x Allows top-up operation ESLS XVIII (25-26/11 2010), Status of the ASTRID2 project 3 ESLS XVIII (25-26/11 2010), Status of the ASTRID2 project 4 ASTRID2 parameters Combined function dipoles 6x2 solid sector Energy 580 MeV Nominal (max.) dipole field 1.1975 (1.25) T Circumference 45.704 m Bending radius 1.62 m Current 200 mA Nominal quadrupole field ‐3.219 T/m Nominal sextupole field ‐8.0 T/m2 Straight sections 4x2.7 m Quadrupoles 6x(2+2) Betatron tunes 5.185, 2.14 Magnetic length 0.132 m Coupling factor <10% Max. gradient 20 T/m Horizontal emittance 12 nm Sextupoles 6x(2+1) Natural chromaticity ‐6, ‐11 Magnetic length 0.170 m Dynamical aperture 25‐30 mm Max. -
Dynamic Aperture Vertical Emittance Control Experiments at PETRA II
PETRA III Beam Dynamics Issues Dynamic Aperture Vertical Emittance Control Experiments at PETRA II 5th DESY MAC, 1.6.2005 Winni Decking, DESY-MPY 5th DESY MAC PETRA III Beam Dynamics Issues Winni Decking - DESY Dynamic Aperture 5th DESY MAC PETRA III Beam Dynamics Issues Winni Decking - DESY Dynamic Aperture • Loss-free injection requires horizontal aperture of 30 mm mrad • Touschek lifetime requires off-momentum aperture of 1.5 % 35 without all insertion devices with all insertion devices 30 25 20 (mm mrad) 15 y A 10 5 0 0 20 40 60 80 100 120 A (mm mrad) x 5th DESY MAC PETRA III Beam Dynamics Issues Winni Decking - DESY Dynamic Aperture Large cross-term due to sextupoles limit horizontal DA Wigglers and Undulators enhance vertical detuning with vertical amplitude Present sextupole scheme: 2 families within 72deg lattice correct chromaticity first order perturbations cancelled after 5 cells d(Qx)/d(Ex) d(Qy)/(dEy) d(Qy)/d(Ex) -4.75E+02 -1.85E+02 -3.30E+03 More sextupole families to tackle cross term? 5th DESY MAC PETRA III Beam Dynamics Issues Winni Decking - DESY PETRA III ‘Symmetries’ Octant (-B) -B C 13 FBDB 2 FODB B D 10 regular FODO cells -B A A -A 5th DESY MAC PETRA III Beam Dynamics Issues Winni Decking - DESY Sextupole Schemes symmetry point 5*(S1,S2) 5*(S1,S2) 5*(S1,S2) 5*(S3,S4) SH1,SH2 5*(S1, S2) 5*( S1,S2) SH3,SH4 5*(S1,S2,S3,S4) β [45m] D [1m] 5th DESY MAC PETRA III Beam Dynamics Issues Winni Decking - DESY Results • Two family scheme further optimized (working point, …) • Non-interleaved four family scheme allows to reduce cross-term. -
Suddenly Saskatchewan Magazine Is for Information Purposes Only
MAGAZINE | SUMMER 2021 Fighting COVID-19 at Canada’s Synchrotron Performance Cycling Program for Youth Arrowhead Helicopter Steel-Craft Door Charter Services MADE IN CANADA Ducks Unlimited Rockglen’s Unique PRESErvING Paleontology SASKAtchEWAN HERITAGE Visit Abode Furniture’s NEW Showroom Royal Saskatchewan Museum & T.REX Discovery Centre SUMMER TOURS WELCOME TO MULBERRy’s! MAGAZINE | SUMMER 2021 Mulberry’s Restaurant & Catering is a Fighting COVID-19 The Canadian Light Source local family owned & operated business at Canada’s Synchrotron that has been serving Saskatoon for over 40 years .We are excited about our Performance Cycling Program for Youth Arrowhead move to our new location at 2326 B Millar Helicopter Steel-Craft Door Charter Services MADE IN CANADA Ave in January 2020, and look forward to Ducks Unlimited Rockglenn’s Unique PRESERVING Paleontology SASKATCHEWAN HERITAGE Visit Abode Furniture’s maintaining our quality dining for you in NEW Showroom our bright and cheery environment. Royal Saskatchewan Museum & T.REX Discovery Centre SUMMER TOURS Whatever your taste, Mulberry’s is sure to Cover photo courtesy: have something for you; whether it is early Canadian Light Source morning breakfast, fresh baked bread, Exciting Things are Happening late night parties and catering for your Copyright & Disclaimer: gatherings. The material distributed in at Mulberry’s on Millar Avenue! the Suddenly Saskatchewan Magazine is for information purposes only. Suddenly he Canadian Light Source (CLS) at the University of Saskatchewan is Saskatchewan Magazine a national research facility, producing the brightest light in Canada— The popular restaurant is becoming “The Fully licensed North assumes no liability or End EVENT Centre.” Mulberry’s broadened facilities and expertise responsibility for any millions of times brighter than even the sun. -
Jørgen S. Nielsen Institute for Storage Ring Facilities (ISA) Aarhus University Denmark
Jørgen S. Nielsen Institute for Storage Ring Facilities (ISA) Aarhus University Denmark ESLS-RF 13 (30/9-1/10 2009), ASTRID2 and its RF system 1 ASTRID2 is the new synchrotron light source to be built in Århus, Denmark Dec 2008: Awarded 5.0 M€ for ◦ Construction of the synchrotron ◦ Transfer of beamlines from ASTRID1 to ASTRID2 ◦ New multipole wiggler ◦ We did apply for 5.5 M€ Cut away an undulator for a new beamline Has to be financed together with a new beamline Saved some money by changing the multipole wiggler to better match our need ESLS-RF 13 (30/9-1/10 2009), ASTRID2 and its RF system 2 ◦ Electron energy: 580 MeV ◦ Emittance: 12 nm ◦ Beam Current: 200 mA ◦ Circumference: 45.7 m ◦ 6-fold symmetry lattice: DBA with 12 combined function dipole magnets Integrated quadrupole gradient ◦ 4 straight sections for insertion devices ◦ Will use ASTRID as booster (full energy injection) Allows top-up operation ESLS-RF 13 (30/9-1/10 2009), ASTRID2 and its RF system 3 ESLS-RF 13 (30/9-1/10 2009), ASTRID2 and its RF system 4 ESLS-RF 13 (30/9-1/10 2009), ASTRID2 and its RF system 5 General parameters ASTRID2 ASTRID Energy E [GeV] 0.58 0.58 Dipole field B [T] 1.192 1.6 Circumference L [m] 45.704 40.00 Current I [mA] 200 200 Revolution time T [ns] 152.45 133.43 Length straight sections [m] ~3 Number of insertion devices 4 1 Lattice parameters Straight section dispersion [m] 0 2.7 Horizontal tune Qx 5.23 2.29 Vertical tune Qy 2.14 2.69 Horizontal chromaticity dQ x/d( ∆p/p) -6.4 -4.0 Vertical chromaticity dQ y/d( ∆p/p) -11.2 -7.1 Momentum -
Progress Report
2013 Progress Report GLOBAL INSTITUTE for FOOD SECURITY POTASHCORP – A FOUNDING PARTNER INVESTING IN GLOBAL FOOD SOLUTIONS: 2013 – A FOUNDATIONAL YEAR THE FOUNDING PARTNERS years, with which the Institute will With a shared vision to develop apply Saskatchewan’s unique resources, Saskatchewan-led solutions to feed a innovation and expertise to address growing world population, the Global the increasing global demand for safe, Institute for Food Security (GIFS) was reliable food. established on December 10, 2012 University of Saskatchewan, a world- through a unique public-private renowned centre of excellence in partnership of PotashCorp, the agriculture and food-system related Government of Saskatchewan and research, contributed its world-class the University of Saskatchewan. facilities and centres of expertise critical PotashCorp provided an initial investment to the Institute’s success. Representatives of the Founding Partners to GIFS of up to CDN $35 million over Through the Institute, Saskatchewan launched the Global Institute for Food Security seven years, which represents the largest will make contributions to global food on December 10, 2012. donation in the company’s history and security by supplying healthy agricultural L to R: reflects its deep commitment to food commodities and food ingredients, as well Bill Doyle, President and CEO, PotashCorp; security. The donation is one of the as crop production inputs such as potash. Dr. Ilene Busch-Vishniac, President, largest corporate donations for university It will be a world leader in innovations University of Saskatchewan; research in Canada. Brad Wall, Premier, Province of Saskatchewan. in agriculture and will be a model for The Government of Saskatchewan international cooperation in science and invested CDN $15 million over seven technology transfer. -
ASTRID2 -The New Low-Emmitance Light Source in Denmark
Proceedings of IPAC’10, Kyoto, Japan WEPEA008 ASTRID2 - THE NEW LOW-EMITTANCE LIGHT SOURCE IN DENMARK S.P. Møller, N. Hertel, and J.S. Nielsen, ISA, Aarhus University, Aarhus, Denmark Abstract Two families of sextupoles are installed to compensate A new low-energy synchrotron radiation light source is and vary chromaticity. Initially, strong sextupole presently being built at Aarhus University. The storage components in the combined-function dipoles were ring will circulate a 580 MeV electron beam with an proposed, but it turned out that such extended strong emittance of 10 nm. Due to the moderate lifetime of a few sextupoles reduced the dynamical aperture drastically [2]. hours, the machine will be operated in top-up mode at 200 After introduction of short sextupoles, the dynamical mA with injection from the present ASTRID storage ring. aperture could be enlarged to a value in excess of the In the present contribution, we will describe aspects of the physical aperture. However, a small negative sextupole lattice, the injection and the expected performance of the component was introduced in the dipoles as this increased machine. the vertical dynamical aperture even further by ~50 %. The main data for ASTRID2 are given in Table 1. INTRODUCTION The lattice will include 24 button pickup systems, 24 horizontal and 12 vertical correction dipoles. The ASTRID storage ring [1] has now been in operation for 20 years, and although the machine at 580 Table 1: ASTRID2 Specifications MeV has a very good lifetime in excess of 100 hours at Quantity Value 150 mA, the relatively large emittance (140 nm), the limited stability and lack of straight sections for insertion Energy 580 MeV devices has since long called for an upgrade. -
Protocol for the Medical Isotope Project
Protocol for the Medical Isotope Project Canadian Light Source Inc. Canadian Nuclear Safety Commission February 2011 CNSC FILE # 2.03 E-Docs #3645315 TABLE OF CONTENTS Summary of Changes .................................................................................................................................... i Extent of the Protocol................................................................................................................................... ii 1. Introduction......................................................................................................................................... 1 2. Objective.............................................................................................................................................. 1 3. Approach to Licensing........................................................................................................................ 1 4. Schedule ............................................................................................................................................... 2 5. Parties and Organizational Representatives..................................................................................... 2 6. Statement of Work.............................................................................................................................. 3 Project requirements.................................................................................................................................... 3 (a) Project description for