Eric Prebys USPAS, Hampton, VA 2015.  Wikipedia lists about 60 light sources worldwide USPAS, Hampton, VA 2015Special Topic - Light Sources 2.

Slides:



Advertisements
Similar presentations
1 Diamond RAL Particle Physics Masterclass 12 March 2003 Glenn Patrick
Advertisements

Eric Prebys, FNAL. USPAS, Knoxville, TN, Jan , 2014 Lecture 13 - Synchrotron Radiation 2 For a relativistic particle, the total radiated power (S&E.
Prajwal Mohanmurthy, Mississippi State University with Dr. Dipangkar Dutta, Mississippi State University Medium Energy Physics Group Spin-Light Polarimeter.
AST 101 Lecture 9 The Light of your Life
Wavelength, Frequency, and Energy Practice Problems
GUINEA-PIG: A tool for beam-beam effect study C. Rimbault, LAL Orsay Daresbury, April 2006.
Linear Collider Bunch Compressors Andy Wolski Lawrence Berkeley National Laboratory USPAS Santa Barbara, June 2003.
R. Nagaoka, A. Nadji, M.E. Couprie, O. Marcouillé
Necessity of Moving from Green Book to White Book M. Hadi Hadizadeh Yazdi International Scientific Meetings Office Iran October 26, 2002 Amman, Jordan.
The Phase-Resolved Spectra of the Crab Pulsar Jianjun Jia Jan 3, 2006.
Professor David Attwood / UC Berkeley / ICTP-IAEA School, Trieste, November 2014 ICTP_Trieste_Lec1_Nov2014.pptx Introduction to Synchrotron Radiation and.
Radiation & Photometry AS4100 Astrofisika Pengamatan Prodi Astronomi 2007/2008 B. Dermawan.
Accelerator Physics: Synchrotron radiation Lecture 2 Henrik Kjeldsen – ISA.
Space Charge Electric-Field Calculations for Coherent Tune Shift Estimations using the Electron-cloud Modelling Algorithm ECLOUD Jim Crittenden Cornell.
CESR Synchrotron Radiation Tables and Electron Cloud Modelling Input Parameters Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education.
Beam Dynamics Tutorial, L. Rivkin, EPFL & PSI, Prague, September 2014 Synchrotron radiation in LHC: spectrum and dynamics The Large Hadron Collider (LHC)
Chapter 2: Particle Properties of Waves
Impact of synchrotron radiation in LEPTON COLLIDER arcs
Prajwal T. Mohan Murthy Laboratory for Nuclear Science, MIT νDM Group Spin-Light Polarimeter for the Electron Ion Collider EIC Users Meeting 2014 Jun 2014.
© 2010 Pearson Education, Inc. Light and Matter: Reading Messages from the Cosmos.
Syllabus and slides Lecture 1: Overview and history of Particle accelerators (EW) Lecture 2: Beam optics I (transverse) (EW) Lecture 3: Beam optics II.
Lecture 1: Synchrotron radiation Lecture 2: Undulators and Wigglers
SESAME Synchrotron Light for Experimental Science and Applications in the Middle East JSPS Asien Science Seminar Synchrotron Radiation Science Dieter Einfeld.
Eric Prebys USPAS, Knoxville, TN, Jan , 2014.
Electromagnetic radiation sources based on relativistic electron and ion beams E.G.Bessonov 1.Introduction 2.Spontaneous and stimulated emission of electromagnetic.
Tools for Nuclear & Particle Physics Experimental Background.
June 14th 2005 Accelerator Division Overview of ALBA D. Einfeld Vacuum Workshop Barcelona, 12 th -13 th September 2005 General 10 th September 2005.
Synchrotron Radiation Sources Past, Present and Future
1/18 The Distribution of Synchrotron Radiation Power in the IR C. H. Yu IR Overview SR Distribution in the IR The Protection of SR Power.
The impact of undulators in an ERL Jim Clarke ASTeC, STFC Daresbury Laboratory FLS 2012, March 2012.
Measurement of Gas Bremsstrahlung at the Pohang Light Source Hyosang Lee Seoul National University, Q2C Pusan National University, HANUL HNP2011.
Properties of Synchrotron Radiation Presentation at JASS02 Seminar; Jordan, Oct , 2002 Herman Winick, SSRL/SLAC, Stanford University.
05/05/2004Cyrille Thomas DIAMOND Storage Ring Optical and X-ray Diagnostics.
PHY418 PARTICLE ASTROPHYSICS Radio Emission 1. Radio emission and particle astrophysics 2 Why are the.
Eric Prebys USPAS, Knoxville, TN, Jan , 2014.
Synchrotron radiation at eRHIC Yichao Jing, Oleg Chubar, Vladimir N. Litvinenko.
Electromagnetic Spectrum. Matter Review All matter is made of A______ Matter exists in different forms or phases. They are.
Introduction to Synchrotron Radiation
The Future of Photon Science and Free-Electron Lasers Ingolf Lindau Lund University and Stanford University MAX-Lab and Synchrotron Light Research KTH,
Eric Prebys, FNAL.  In our previous discussion, we implicitly assumed that the distribution of particles in phase space followed the ellipse defined.
“Physics and the Quantum Mechanical Model” Read pg. 138 p. 1
Main Bullet #1 Main Bullet #2 Main Bullet #3 Advances in Coherent Synchrotron Radiation at the Canadian Light Source Jack Bergstrom.
Lighting the path to innovation Australian Synchrotron What is a synchrotron & how does it work?
Synchrotron Radiation
ELECTRON MOVING AT CONSTANT VELOCITY
ELECTROMAGNETIC SPECTRA. c = λν E = hν E = mc 2 c = 3.00 x 10 8 m / sec h = x J sec Hz = 1 / sec HELPFUL EQUATIONS.
Initial (FLUKA) calculations for synchrotron radiation at TLep April 4 th, 2013 F. Cerutti, A. Ferrari, L. Lari* *BE Dept.
USPAS Course on Recirculated and Energy Recovered Linacs G. A. Krafft and A. Bogacz Jefferson Lab Timofey Zolkin Lecture 12: ERL x-ray light source USPAS.
Adams Accelerator Institute 10 - E. Wilson - 1/24/ Slide 1 Lecture 14 ACCELERATOR PHYSICS MT 2004 E. J. N. Wilson.
11. Radiation. What is radiation? Radiation sources Antenna: radio waves, microwaves Atoms, molecules: light, infrared light, UV, X-rays Nuclei: Gamma.
Workshop on Accelerator R&D for Ultimate Storage Rings – Oct Nov.1 – Huairou, Beijing, China A compact low emittance lattice with superbends for.
Synchrotron Radiation Lecture 1 Introduction to Synchrotron Radiation Jim Clarke ASTeC Daresbury Laboratory.
Eric Prebys, FNAL. USPAS, Ft. Collins, CO June 13-24, 2016 E. Prebys - Accelerator Fundamentals, Synchrotron Radiation 2 For a relativistic particle,
EMS (ELECTRO MAGNETIC SPECTRUM). WHAT TYPES OF RADIATION (WAVES) ARE NOT VISIBLE? CAN YOU RANK THEM IN ORDER OF ENERGY? (WHICH ARE MORE ENERGETIC)?
Jim Clarke STFC Daresbury Laboratory, UK & The Cockcroft Institute, UK
Rutherford Model Know where the protons and neutrons are, but where are the electrons? If opposite charges attract, why do the electrons not fall into.
Very Asymmetric Collider for Dark Matter Search below 1 GeV
II. Bohr Model of the Atom (p )
Free Electron Lasers (FEL’s)
Lecture 15 ACCELERATOR PHYSICS MT 2004 E. J. N. Wilson.
Waves and Electromagnetic Radiation
Специализированный источник синхротронного излучения Anka Характеристики и экспериментальные возможности.
Coherent Synchrotron Radiation Study
Accelerator Physics NMI and Synchrotron Radiation
Radiation Damping - Low emittance lattices
Accelerator Physics Synchrotron Radiation
USPAS Course on 4th Generation Light Sources II
USPAS Course on 4th Generation Light Sources II
MEIC Alternative Design Part V
Electron Rings 2 Eduard Pozdeyev.
Presentation transcript:

Eric Prebys USPAS, Hampton, VA 2015

 Wikipedia lists about 60 light sources worldwide USPAS, Hampton, VA 2015Special Topic - Light Sources 2

 Bending electrons emit radiation along their path USPAS, Hampton, VA 2015Special Topic - Light Sources 3

 Synchrotron Radiation was first searched for in 1944 at GE’s 100 MeV electron accelerator.  Energy loss was seen, but because of a calculational error, they searched in the microwave region and missed the visible light, because the acceleration chamber was opaque  In 1947, John Paul Blewett got permission to build a 70 MeV cyclotron at GE with transparent windows, and observed synchrotron radiation for the first time. USPAS, Hampton, VA 2015Special Topic - Light Sources 4

 Examples  SURF (1961): 180 MeV UV synchrotron at NBS  CESR (CHESS, 70’s): 6 GeV synchrotron at Cornell  Numerous others  Typically large emittances, which limited brightness of the beam USPAS, Hampton, VA 2015Special Topic - Light Sources 5

 Examples:  1981: 2 GeV SRS at Daresbury(  =106 nm-rad)  1982: 800 MeV BESSY in Berlin(  =38 nm-rad)  1990: SPEAR II becomes dedicated light source(  =160 nm-rad)  Often include “wigglers” to enhance SR USPAS, Hampton, VA 2015Special Topic - Light Sources 6

 Beam sizes   y ~1 mm   y’ ~.1 mrad   x ~.1 mm   x‘ ~.03 mrad  Broad spectrum  High flux  Typically photons/second/mradian for 3 GeV, 100 mA dipole source at E crit USPAS, Hampton, VA 2015Special Topic - Light Sources 7

 In rest frame of electron  Electron oscillates coherently with (contracted) structure, and releases photons with the same wavelength.  In the lab frame, this is Doppler shifted, so  So, on the order of 1cm  X-rays. USPAS, Hampton, VA 2015Special Topic - Light Sources 8 Periodic Magnets

USPAS, Hampton, VA 2015Special Topic - Light Sources 9 *G. Krafft

 High Brightness  compared to for 2 nd generation sources  Emittance ~1-20 nm-rad USPAS, Hampton, VA 2015Special Topic - Light Sources 10

USPAS, Hampton, VA 2015Special Topic - Light Sources 11