DOCSLIB.ORG

Undulator Radiation & FEL

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
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 Undulators L0 X-rays electrons Layout of the sub-systems of the LCLS first X-ray FEL 5 Linac Coherent Light Source LCLS-II LCLS-II-HE Photoinjector The last 1 km of the SLAC linac accelerates electrons up to 15 GeV Starting at Sector 20, electron bunches are Linac-to-Undulator Transport (340m) injected at 135 MeV 140-m long undulator hall with 2 side-by-side undulators, Hard X-ray (HXR) and Soft X-ray (SXR) Near Experimental Hall Far Experimental Hall 6 RF-linac Driven FEL Pulse Format Low-repetition-rate Mode (e.g., LCLS CuRF) ~8 ms (1/120 Hz) ~10 fs Burst Mode (e.g., Eu-XFEL) ~1 ms macropulse ~1 ms macropulse ~100 ms (1/10 Hz) ~200ns micropulses Continuous-Wave Mode (e.g., LCLS-II/HE, SHINE) ~1 ms (1/MHz) 7 LCLS-II-HE Soft X-ray Undulator Planar Undulators strongback magnetic field electron beam magnets 푢 X-ray polarization (same direction as Undulator magnetic field varies sinusoidally electron oscillations) with z and points in the y direction B = 퐵0푠푖푛 푘푢푧 풚ෝ Planar undulators produce linearly (plane) polarized radiation at the fundamental frequency and also at harmonic frequencies. 8 Helical Superconducting Undulators Superconducting coils are wound around the electron beam pipe in a helical pattern. Undulator magnetic field varies sinusoidally with z and points in both x and y directions in a helical fashion. B = 퐵0 푐표푠 푘푢푧 풙ෝ + 푠푖푛 푘푢푧 풚ෝ 2휋 Undulator wavenumber 푘푢 = 푢 Helical undulators produce circularly Snapshots of the helical polarized radiation at the fundamental undulator magnetic field at frequency. Helical undulators do not different locations in one produce undulator radiation at the undulator period. harmonic frequencies. 9 Delta Undulators (Variable Polarization) Varying the linear positions of the magnet jaws Delta undulator cross-section changes radiation polarization from linear to circular 10 X-ray FEL Wavelength for a Planar Undulator Undulator period FEL resonant wavelength 2 푢 퐾 Undulator parameter = 2 1 + 2훾 2 푒퐵0 푒푢퐵0 K = = Lorentz relativistic factor 푘 푚 푐 2휋푚 푐 (Dimensionless beam energy) 푢 푒 푒 Dimensionless K parameter is a measure 퐸푡표푡푎푙 of how much the electron beam is K = 0.934 퐵 훾 = 2 0 푢 푚푒푐 deflected transversely in the undulator 퐾 휃푚푎푥 = 푥 훾 B0 in tesla 푢 in cm radiation wave u + 휃푚푎푥 푧 e- trajectory u 11 Electron Beam Kinematics Dimensionless electron beam energy Electron velocity relative to the speed of light 푣 퐸푡표푡푎푙 훽 = 훾 = 2 푐 푚푒푐 Using the g-b relation, we can calculate b 2 퐸푡표푡푎푙 = 퐸푘 + 푚푒푐 1 1 훾 = 훽 = 1 − 1 − 훽2 2 Rest mass energy 훾 Kinetic energy 0.511 MeV Approximate b for 1 Approximate g for GeV electrons GeV electrons 훽 ≈ 1 − 2훾2 퐸푡표푡푎푙 ≈ 퐸푘 = 퐸푏 We shall see later the longitudinal component of 훾 ≈ 1957 퐸푏 퐺푒푉 the velocity, ʋz is reduced when the electrons undergo transverse oscillations in the undulator. 12 X-ray FEL Wavelength Tuning The FEL x-ray wavelength can be tuned by one of the following methods 1. varying the electron beam energy, Eb and thus the beam g 2. varying the gap by moving the magnet jaws symmetrically in and out, thus changing the K value 2 The on-axis magnetic field amplitude depends 푔 푔 on the gap-to-period ratio. The remanence 퐵0 푔, 푢 = 3.13퐵푟 푒푥푝 −5.08 + 1.54 푢 푢 magnetic field, 퐵 푟 of NdFeB is about 1.2 tesla. Small gap – Large K – Long Larger gap – Smaller K – Shorter gap gap e- beam e- beam poles magnets period 13 LCLS-II-HE Variable-Gap Soft X-ray Undulator SXR K parameterK vs gap (mm) This example illustrates how we change the LCLS X-ray FEL 10 9 wavelength by varying the magnet gap of the Soft X-ray 8 (SXR) undulator which has an undulator period of 56 mm. 7 6 The undulator K parameter decreases and photon energy K 5 4 increases as we increase the gap (right figures), using the 3 LCLS-II-HE 8-GeV electron beams as an example. 2 1 However, opening the gap to increase the photon energy 0 also reduces the FEL output pulse energy (below). 7.2 9.2 11.2 13.2 15.2Photon17.2 19.2 energy21.2 23.2 25.2 27.2 29.2 31.2 5000 3.5 4500 Photon energy (eV) vs gap (mm) 3 4000 2.5 3500 3000 Output 2 Photon 2500 pulse 1.5 energy energy (eV) 2000 1 (mJ) 1500 0.5 1000 0 500 500 750 250 0 1250 1500 1750 2000 2250 2500 2750 3000 3250 3500 3750 4000 4250 4500 4750 5000 5000 1000 7.2 9.2 11.2 13.2 15.2 17.2 19.2 21.2 23.2 25.2 27.2 29.2 31.2 Photon energy (eV) 14 gap (mm) Properties of Electromagnetic Radiation 15 EM Radiation in Free Space ℎ = 4.1357 ∙ 10−15 푒V ∙ 푠 푐 = 2.9979 ∙ 108 푚/푠 Low frequency Long wavelength ∙ ℎ휈 = ℎ푐 = 1.23984 ∙ 10−6푒V−m 1239.84 푒푉 Photon energy ℎ휈 = λ 푛푚 푥 푐 푦 푧 High frequency Short wavelength 16 Accelerated charged particles emit EM radiation Radiation from circular motions Bremsstrahlung Synchrotron radiation Radiation from oscillatory motions 17 Generations of Beam-based Radiation Sources • X-ray Tubes – X-ray tubes emit Bremsstrahlung and characteristic peaks – Characteristic peaks are narrow-line atomic transitions • Synchrotron Radiation (1st and 2nd Generation Light Sources) – Electrons going around bends produce synchrotron radiation – First generation SR operated as parasitic radiation devices – Second generation SR are dedicated to radiation production • Synchrotron Radiation (3rd Generation Light Sources) – 3rd Gen SR have low-emittance lattice with straight sections – Bending magnet and wiggler radiation is broadband – Undulator radiation has narrow spectral lines • X-ray Free-Electron Lasers (4th Generation Light Sources) – XFEL produce coherent, tunable, narrow-band x-rays – X-ray pulses are typically a few femtoseconds long – FEL peak brilliance is typically 10 orders of magnitude brighter than third-generation SR. 18 Electric Field of a Gaussian Wave-Packet Complex electric 푡−푡 2 − 0 field of a Gaussian 2 퐸(푧, 푡) = 퐸 푒 푘푧−휔푡+휓 푒 2휎푡 wave-packet 0 + c.c. Amplitude Phase Gaussian envelope rms temporal width Wavenumber Angular frequency 2휋 2휋푐 Radiation intensity 푘 = 휔 = 1 퐼 = 퐸 푧, 푡 2 2푍0 Normalized Fast carrier waves at w intensity envelope 1 2 퐼0 = 퐸0 2푍0 Gaussian envelope Impedance of free space = 120p 19 Fourier Transform a Gaussian Pulse Consider only the time-dependent part of a 푡2 Gaussian wave-packet. Its Fourier Transform 퐸0 − 2 ℰ(휔) = න 푒− 휔−휔푟 푡푒 2휎푡 푑푡 is a Gaussian spectrum centered at ± 휔푟 2휋 2 2 푡 휔−휔푟 − 2 퐸0 − 2 −휔푟푡 2휎 ℰ(휔) = 2휎휔 퐸(푡) = 퐸0푒 푒 푡 푒 2휎휔 Fourier Transform limit 2휎푡 of time-bandwidth product (rms widths) ℰ 휔 2 휎휔휎푡 = ½ 2휎휔 In general, TBW is larger than 1/2 휔푟 Time domain Frequency domain 20 Radiation Pulse & Time-Bandwidth Product Linear frequency Full-width-at-half-maximum (FWHM) in FWHM time 훿 푡 and linear frequency domain 훿휈 휔 휈 = 2휋 • Time-bandwidth product for a Gaussian pulse 2 4푙푛2 퐸 푡 d푡 훿휈 ∙ 훿푡 = 휎 휎 = 0.44 훿푡 = 2 2푙푛2 휎 휋 휔 푡 푡 • Multiply both sides by the Planck’s constant in eV-s -4.0 -3.0 -2.0 -1.0 0.0 1.0 2.0 3.0 4.0 푡 − 푡0 ℎ = 4.136 ∙ 10−15 푒V-s 휎휔 ℎ훿휈 ∙ 훿푡 = 1.82 푒푉 ∙ 푓푠 훿휈 = 2 2푙푛2 2휋 훿휈 Energy (eV) – time FWHM product ℰ 휈 2 훿휀 ∙ 훿푡 ≥ 1.82 푒푉 ∙ 푓푠 휈 − 휈푟 21 Wave Equation & Helmholtz Equation • Wave equation 1 휕2 2 − 푢 풓, 푡 = 0 푐2 휕푡2 −휔 푡 • Solution to the wave equation 푢 풓, 푡 = Re 풓 푒 푟 Time-independent Time-dependent wave amplitude oscillatory term • Helmholtz equation for the time-independent wave amplitude 2 + 푘2 풓 = 0 풓 = 퐴 풓 푒풌·풓 22 Paraxial Approximation Paraxial wave equation for a wave 2 휕 propagating in the z direction 푇 − 2푖푘 퐴 푥, 푦, 푧 = 0 휕푧 Gaussian beam transverse amplitude T denotes transverse spreading due (beam propagating in the z direction) to optical diffraction 휕2 휕2 2 = + 2 2 2 푇 2 2 and 푘 = 푘푥 + 푘푦 + 푘푧 휕푥 휕푦 2 2 2 Paraxial approximation 푘푥 + 푘푦 ≪ 푘푧 푦 For axisymmetric Gaussian beams, 푘푥 = 푘푦 푟2 푟2 푤 − 푘 퐸(푟, 푧) = 퐸 0 푒 푤2 푧 푒 푘푧−휔푡+휓 푧 푒 2푅 푧 0 푤 푧 푥 Gouy phase shift 푤0 is the radius where the field Radius of curvature of the decays to 1/e of E0 at the beam waist 푤 푧 z Gaussian beam wavefront is the 1/e radius at location 23 Gaussian Beam Intensity & Diffraction 퐼 • 1 0 Optical intensity 퐼 푟, 푧 = 퐸 푟, 푧 2 2푍0 2푟2 퐼 푟 • Gaussian beam 푤 2 − 0 푒 푤2 퐼(푟, 푧) = 퐼0 푤0 푤 퐼0 푧2 푒2 푤 = 푤0 1 + 2 -4.0 -3.0 -2.0 -1.0 0.0
Load more

Recommended publications
  • 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.
    [Show full text]
  • 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
    [Show full text]
  • 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
    [Show full text]
  • 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.
    [Show full text]
  • Electron Beam Brightness and Undulator Radiation Brilliance for a Laser Plasma Acceleration Based Free Electron Laser
    instruments Article Electron Beam Brightness and Undulator Radiation Brilliance for a Laser Plasma Acceleration Based Free Electron Laser Amin Ghaith 1,* , Alexandre Loulergue 1, Driss Oumbarek 1, Olivier Marcouillé 1, Mathieu Valléau 1, Marie Labat 1, Sebastien Corde 2 and Marie-Emmanuelle Couprie 1 1 Synchrotron Source Optimisée de Lumière d’Energie Intermédiaire du LURE (Laboratoire pour l’Utilisation du Rayonnement Electromagnétique) (Synchrotron SOLEIL), L’Orme des Merisiers, 91190 Saint-Aubin, France; alexandre.loulergue@synchrotron-soleil.fr (A.L.); driss.oumbarek-espinos@synchrotron-soleil.fr (D.O.); olivier.marcouille@synchrotron-soleil.fr (O.M.); mathieu.valleau@synchrotron-soleil.fr (M.V.); marie.labat@synchrotron-soleil.fr (M.L.); marie-emmanuelle.couprie@synchrotron-soleil.fr (M.-E.C.) 2 École Nationale Supérieure de Techniques Avancées Paris (ENSTA Paris), Centre National de la Recherche Scientifique (CNRS), Ecole Polytechnique, Institut Polytechnique de Paris, 91128 Palaiseau, France; sebastien.corde@polytechnique.edu * Correspondence: amin.ghaith@synchrotron-soleil.fr Received: 3 December 2019; Accepted: 27 December 2019; Published: 1 January 2020 Abstract: We report here on spontaneous undulator radiation and free electron laser calculations after a 10-m long transport line (COXINEL) using a Laser Plasma acceleration (LPA) source. The line enables the manipulation of the properties of the produced electron beams (energy spread, divergence, dispersion) in view of light source applications. The electron beam brightness and undulator radiation brilliance are addressed by an analytical approach enabling us to point out the influence of chromatic effects in the COXINEL case. Keywords: laser plasma acceleration; electron beam brightness; undulator radiation; free electron laser 1. Introduction Particle accelerators have become a crucial need for advancement in many domains such as nanotechnology, atomic physics, nuclear physics, chemistry and medicine.
    [Show full text]
  • Lecture - Day 8
    Fundamentals of Accelerators - 2012 Lecture - Day 8 William A. Barletta Director, US Particle Accelerator School Dept. of Physics, MIT Economics Faculty, University of Ljubljana US Particle Accelerator School What do we mean by radiation? Energy is transmitted by the electromagnetic field to infinity Applies in all inertial frames Carried by an electromagnetic wave Source of the energy Motion of charges US Particle Accelerator School Schematic of electric field From: T. Shintake, New Real-time Simulation Technique for Synchrotron and Undulator Radiations, Proc. LINAC 2002, Gyeongju, Korea US Particle Accelerator School Static charge US Particle Accelerator School Particle moving in a straight line with constant velocity E field Q B field US Particle Accelerator School Consider the fields from an electron with abrupt accelerations At r = ct, ∃ a transition region from one field to the other. At large r, the field in this layer becomes the radiation field. US Particle Accelerator School Particle moving in a circle at constant speed dQ = q dl Field energy flows to infinity US Particle Accelerator School Remember that fields add, we can compute radiation from a charge twice as long dQ = 2q dl The wavelength of the radiation doubles US Particle Accelerator School All these radiate Not quantitatively correct because E is a vector; But we can see that the peak field hits the observer twice as often US Particle Accelerator School Current loop: No radiation Field is static B field US Particle Accelerator School QED approach: Why do particles radiate when accelerated? Charged particles in free space are “surrounded” by virtual photons Appear & disappear & travel with the particles.
    [Show full text]
  • The Free Electron Laser Klystron Amplifier Concept
    E.L. Saldin et al. / Proceedings of the 2004 FEL Conference, 143-146 143 THE FREE ELECTRON LASER KLYSTRON AMPLIFIER CONCEPT E.L. Saldin, E.A. Schneidmiller, and M.V. Yurkov Deutsches Elektronen-Synchrotron (DESY), Hamburg, Germany Abstract as short as 10-100 µm have never been measured and are challenging to predict. We consider optical klystron with a high gain per cas- The situation is quite different for klystron amplifier cade pass. In order to achieve high gain at short wave- scheme described in our paper. A distinguishing feature of lengths, conventional FEL amplifiers require electron beam the klystron amplifier is the absence of apparent limitations peak current of a few kA. This is achieved by applying which would prevent operation without bunch compression longitudinal compression using a magnetic chicane. In in the injector linac. As we will see, the gain per cas- the case of klystron things are quite different and gain of cade pass is proportional to the peak current and inversely klystron does not depend on the bunch compression in the proportional to the energy spread of the beam. Since the injector linac. A distinguishing feature of the klystron am- bunch length and energy spread are related to each other plifier is that maximum of gain per cascade pass at high through Liouville’s theorem, the peak current and energy beam peak current is the same as at low beam peak cur- spread cannot vary independently of each other in the injec- rent without compression. Second important feature of the tor linac. To extent that local energy spead is proportional klystron configuration is that there are no requirements on to the peak current, which is usually the case for bunch the alignment of the cascade undulators and dispersion sec- compression, the gain will be independent of the actual tions.
    [Show full text]
  • Optical Klystrons P
    OPTICAL KLYSTRONS P. Elleaume To cite this version: P. Elleaume. OPTICAL KLYSTRONS. Journal de Physique Colloques, 1983, 44 (C1), pp.C1- 333-C1-352. <10.1051/jphyscol:1983127>. <jpa-00222556> HAL Id: jpa-00222556 https://hal.archives-ouvertes.fr/jpa-00222556 Submitted on 1 Jan 1983 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL,est archive for the deposit and dissemination of sci- destin´ee au d´epˆotet `ala di↵usion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publi´es ou non, lished or not. The documents may come from ´emanant des ´etablissements d’enseignement et de teaching and research institutions in France or recherche fran¸cais ou ´etrangers, des laboratoires abroad, or from public or private research centers. publics ou priv´es. JOURNAL DE PHYSIQUE Colloque Cl, supplément au n°8, Tome 44, février 1983 page Cl-333 OPTICAL KLYSTRONS P. Elleaume Département de Physico-Chimie, CEN Saolay, 91191 Gif-sur-Yvette, France Résumé : Le klystron optique est une version modifiée de l'onduleur utilisé pour améliorer le gain du Laser à Electrons Libres. L'émission spontanée et le gain sont calculés en fonction de l'énergie des électrons et de la longueur d'onde. Quelques effets limitant l'augmentation du gain sont étudiés : d i s p e r s i o n en énergie, dispersion angulaire, tailles transverses du faisceau d'électrons. Je discute brièvement l'utilisation de la modulation en densité introduite par le klystron optique sur le faisceau d'électrons pour générer du rayonnement synchrotron cohérent.
    [Show full text]
  • A New PLS-II In-Vacuum Undulator and Characterization Of
    A New PLS-II In-Vacuum Undulator and Characterization of Undulator Radiation D-E. Kim, H-H. Lee, K-H. Park, H-S. Seo, T. Ha, Y-G. Jeong, H-S. Han, W.W. Lee, J-Y. Huang, S. Nam, K-R. Kim and S. Shin Pohang Accelerator Laboratory, POSTECH, Pohang, 790-784, KOREA This paper describes the result of overall studies from development to characterization of undulator radiation. After three years of upgrading, PLS-II [1, 2] has been operating successfully since 21st March 2012. During the upgrade, we developed and installed an in-vacuum undulator (IVU) that generates brilliant X-ray beam. The IVU with 3 GeV electron beam generates undulator radiation up to ~ 21 keV using 11th higher harmonic. The characterizations of the undulator radiation at an X-ray beam line in PLS-II agreed well with the simulation. Based on this performance demonstration, the in-vacuum undulator is successfully operating at PLS-II. PACS number: 07-85-Qe Keywords: Synchrotron radiation, Undulator, X-ray beamline Email: tlssh@postech.ac.kr Fax: +82-54-279-1799 1 I. INTRODUCTION Newer generation light sources with medium electron energy around 3 GeV as well as SASE-FEL are adopting in-vacuum undulator (IVU) to obtain short-wavelength and high-brilliance X-rays from undulator with short magnet period and required magnetic field. Pohang Accelerator Laboratory (PAL) [3] had developed IVU during PLS-II project. With operating experience of in-vacuum revolver undulator from SPring-8 [4] and conventional IVU from ADC [5] at the PLS [6], the new IVU with 20 mm magnetic period and 1.8 m long undulator length was developed and have been operated in PLS-II.
    [Show full text]
  • Optical Klystron Enhancement to Self Amplified Spontaneous Emission At
    hv photonics Article Optical Klystron Enhancement to Self Amplified Spontaneous Emission at FERMI Giuseppe Penco 1,*, Enrico Allaria 1, Giovanni De Ninno 1,2, Eugenio Ferrari 1,3 , Luca Giannessi 1,4, Eléonore Roussel 1 and Simone Spampinati 1 1 Elettra-Sincrotrone Trieste S.C.p.A., Strada Statale 14-km 163.5 in AREA Science Park, Basovizza, 34149 Trieste, Italy; enrico.allaria@elettra.eu (E.A.); giovanni.deninno@elettra.eu (G.D.N.); eugenio.ferrari@psi.ch (E.F.); luca.giannessi@elettra.eu (L.G.); eleonore.roussel@elettra.eu (E.R.); simone.spampinati@elettra.eu (S.S.) 2 Laboratory of Quantum Optics, University of Nova Gorica, 5001 Nova Gorica, Slovenia 3 Paul Scherrer Institut, 5232 Villigen, Switzerland 4 Enea, via Enrico Fermi 45, Frascati, 00044 Roma, Italy * Correspondence: giuseppe.penco@elettra.eu Received: 1 February 2017; Accepted: 23 February 2017; Published: 1 March 2017 Abstract: The optical klystron enhancement to a self-amplified spontaneous emission free electron laser has been studied in theory and in simulations and has been experimentally demonstrated on a single-pass high-gain free electron laser, the FERMI FEL-1, in 2014. The main concept consists of two undulators separated by a dispersive section that converts the energy modulation induced in the first undulator in density modulation, enhancing the coherent harmonic generation in the first part of the second undulator. This scheme could be replicated in a multi-stage: the bunching is enhanced after each dispersive section, consistently reducing the saturation length. We have applied the multi-stage optical klystron (OK) scheme on the FEL-2 line at FERMI, whose layout includes three dispersive sections.
    [Show full text]
  • 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
    [Show full text]
  • Small Signal Bi-Period Harmonic Undulator Free Electron Laser
    Progress In Electromagnetics Research C, Vol. 105, 217–227, 2020 Small Signal Bi-Period Harmonic Undulator Free Electron Laser Ganeswar Mishra*, Avani Sharma, and Saif M. Khan Abstract—In this paper, we discuss the spectral property of radiation of an electron moving in a bi- period harmonic undulator field with a phase between the primary undulator field and the harmonic field component. We derive the expression for the photons per second per mrad2 per 0.1% BW of the radiation. A small signal gain analysis also is discussed highlighting this feature of the radiation. A bi-period index parameter, i.e., Λ is introduced in the calculation. According to the value of the index parameter, the scheme can operate as one period or bi-period undulator. It is shown that when Λ = π, the device operates at the fundamental and the third harmonic. However, when Λ = π/2, it is possible to eliminate the third harmonic. 1. INTRODUCTION Insertion devices are the key components of the synchrotron radiation and free electron laser sources. There are interests and technology upgrades of undulator technology for synchrotron radiation source (SRS) and free electron laser (FEL) for producing tunable electromagnetic radiation over the desired electromagnetic spectrum [1–12]. In the synchrotron radiation source, the relativistic electron beam propagates in the magnetic undulator field and emits spontaneous radiation. In the free electron laser scheme, the relativistic electron beam exchanges the kinetic energy to a co-propagating radiation field at the resonant frequency. Most insertion devices are undulators designed either as pure permanent magnet or hybrid permanent magnet according to Halbach field configuration.
    [Show full text]