Micro-bunching: Longitudinal Bunch Profile Measurements at TTF

Similar documents
EFFECTS OF FRINGING FIELDS ON SINGLE PARTICLE DYNAMICS. M. Bassetti and C. Biscari INFN-LNF, CP 13, Frascati (RM), Italy

The evolution of the phase space density of particle beams in external fields

High Brightness Electron Beams Introduction to the physics of high-quality electron beams

The geometric construction of Ewald sphere and Bragg condition:

1 Spherical multipole moments

CHAPTER IV RADIATION BY SIMPLE ACOUSTIC SOURCE. or by vibratory forces acting directly on the fluid, or by the violent motion of the fluid itself.

COLLISIONLESS PLASMA PHYSICS TAKE-HOME EXAM

1) Consider an object of a parabolic shape with rotational symmetry z

MAGNETIC FIELD INTRODUCTION

A moving charged particle creates a magnetic field vector at every point in space except at its position.

Observation of Coherent OTR at LCLS. Unexpected Physics in Standard Beam Diagnostics

Question 1: The dipole

Introduction to Accelerator Physics

Simulation of the Trickle Heating Effect

Collaborative ASSIGNMENT Assignment 3: Sources of magnetic fields Solution

11) A thin, uniform rod of mass M is supported by two vertical strings, as shown below.

q r 1 4πε Review: Two ways to find V at any point in space: Integrate E dl: Sum or Integrate over charges: q 1 r 1 q 2 r 2 r 3 q 3

This gives rise to the separable equation dr/r = 2 cot θ dθ which may be integrated to yield r(θ) = R sin 2 θ (3)

Solving Problems of Advance of Mercury s Perihelion and Deflection of. Photon Around the Sun with New Newton s Formula of Gravity

Solutions. V in = ρ 0. r 2 + a r 2 + b, where a and b are constants. The potential at the center of the atom has to be finite, so a = 0. r 2 + b.

Qualifying Examination Electricity and Magnetism Solutions January 12, 2006

Cancellation of RF Coupler-Induced Emittance Due to Astigmatism

Magnetic Field of a Wire

ANTENNAS. Vector and Scalar Potentials. Maxwell's Equations. D = εe. For a linear, homogeneous, isotropic medium µ and ε are contant.

Physics 161 Fall 2011 Extra Credit 2 Investigating Black Holes - Solutions The Following is Worth 50 Points!!!

, and the curve BC is symmetrical. Find also the horizontal force in x-direction on one side of the body. h C

3. Electromagnetic Waves II

Rydberg-Rydberg Interactions

Magnetic Field. Conference 6. Physics 102 General Physics II

Mechanics Physics 151

Physics 2020, Spring 2005 Lab 5 page 1 of 8. Lab 5. Magnetism

Designing a Sine-Coil for Measurement of Plasma Displacements in IR-T1 Tokamak

1D2G - Numerical solution of the neutron diffusion equation

Electrostatics (Electric Charges and Field) #2 2010

SIO 229 Gravity and Geomagnetism. Lecture 6. J 2 for Earth. J 2 in the solar system. A first look at the geoid.

Chapter 12: Kinematics of a Particle 12.8 CURVILINEAR MOTION: CYLINDRICAL COMPONENTS. u of the polar coordinate system are also shown in

Magnetohydrodynamics (MHD) I

Physics 181. Assignment 4

Making an Exotic Beam with MARS : Part 1. Brian Roeder Cyclotron Institute Texas A&M Univ. 22 June 2009

Phys101 Lectures 30, 31. Wave Motion

Module 05: Gauss s s Law a

Physics: Work & Energy Beyond Earth Guided Inquiry

Electromagnetic Theory 1

Module 9: Electromagnetic Waves-I Lecture 9: Electromagnetic Waves-I

PHYS 110B - HW #7 Spring 2004, Solutions by David Pace Any referenced equations are from Griffiths Problem statements are paraphrased

[Griffiths Ch.1-3] 2008/11/18, 10:10am 12:00am, 1. (6%, 7%, 7%) Suppose the potential at the surface of a hollow hemisphere is specified, as shown

Chapter 13 Gravitation

$ i. !((( dv vol. Physics 8.02 Quiz One Equations Fall q 1 q 2 r 2 C = 2 C! V 2 = Q 2 2C F = 4!" or. r ˆ = points from source q to observer

But for simplicity, we ll define significant as the time it takes a star to lose all memory of its original trajectory, i.e.,

Graphs of Sine and Cosine Functions

CBN 98-1 Developable constant perimeter surfaces: Application to the end design of a tape-wound quadrupole saddle coil

Objects usually are charged up through the transfer of electrons from one object to the other.

Optics for Soft X-ray Seeding of LCLS-II - Grating and Mirrors

Vainshtein mechanism in second-order scalar-tensor theories

University of Illinois at Chicago Department of Physics. Electricity & Magnetism Qualifying Examination

Homework # 3 Solution Key

Chapter 2 Classical propagation

AY 7A - Fall 2010 Section Worksheet 2 - Solutions Energy and Kepler s Law

Multipole Radiation. February 29, The electromagnetic field of an isolated, oscillating source

- 5 - TEST 1R. This is the repeat version of TEST 1, which was held during Session.

AH Mechanics Checklist (Unit 2) AH Mechanics Checklist (Unit 2) Circular Motion

A 1. EN2210: Continuum Mechanics. Homework 7: Fluid Mechanics Solutions

Look over Chapter 22 sections 1-8 Examples 2, 4, 5, Look over Chapter 16 sections 7-9 examples 6, 7, 8, 9. Things To Know 1/22/2008 PHYS 2212

LECTURE 15. Phase-amplitude variables. Non-linear transverse motion

Physics NYB problem set 5 solution

Physics 2B Chapter 22 Notes - Magnetic Field Spring 2018

Physics 506 Winter 2006 Homework Assignment #9 Solutions

Dynamics of Rotational Motion

Module 18: Outline. Magnetic Dipoles Magnetic Torques

1.2 Differential cross section

m1 m2 M 2 = M -1 L 3 T -2

Ch 30 - Sources of Magnetic Field! The Biot-Savart Law! = k m. r 2. Example 1! Example 2!

Paramagnetic spin pumping with microwave magnetic fields

Basic properties of X- rays and neutrons

Magnetic field due to a current loop.

16.1 Permanent magnets

Phys-272 Lecture 17. Motional Electromotive Force (emf) Induced Electric Fields Displacement Currents Maxwell s Equations

( ) Make-up Tests. From Last Time. Electric Field Flux. o The Electric Field Flux through a bit of area is

Fundamentals of Photonics Bahaa E. A. Saleh, Malvin Carl Teich

6.4 Period and Frequency for Uniform Circular Motion

Three-dimensional systems with spherical symmetry

Motions and Coordinates

Describing Circular motion


Faraday s Law. Faraday s Law. Faraday s Experiments. Faraday s Experiments. Magnetic Flux. Chapter 31. Law of Induction (emf( emf) Faraday s Law

Introduction to Accelerators

F Q E v B MAGNETOSTATICS. Creation of magnetic field B. Effect of B on a moving charge. On moving charges only. Stationary and moving charges

Class 2. Lesson 1 Stationary Point Charges and Their Forces. Basic Rules of Electrostatics. Basic Rules of Electrostatics

Sources of Magnetic Fields (chap 28)

Section 8.2 Polar Coordinates

1 Fundamental Solutions to the Wave Equation

Galilean Transformation vs E&M y. Historical Perspective. Chapter 2 Lecture 2 PHYS Special Relativity. Sep. 1, y K K O.

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 10 Solutions. r s

Hopefully Helpful Hints for Gauss s Law

3-7 FLUIDS IN RIGID-BODY MOTION

Lecture 2: Basic plasma equations, self-focusing, direct laser acceleration

r cos, and y r sin with the origin of coordinate system located at

( n x ( ) Last Time Exam 3 results. Question. 3-D particle in box: summary. Modified Bohr model. 3-D Hydrogen atom. r n. = n 2 a o

Electron Density Distribution in HSX

Unit 6 Practice Test. Which vector diagram correctly shows the change in velocity Δv of the mass during this time? (1) (1) A. Energy KE.

Transcription:

Shot Pulses in Rings Mico-bunching: Longitudinal Bunch Pofile Measuements at TTF ) The time vaying fields in a tansvese mode cavity kick the font of a bunch up, and the back of the bunch don. ) A betaton phase advance of π late, the bunch adiates in an undulato 3) The vetical photon angles ae coelated ith the souce point Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

Shot Pulses in Rings Mico-bunching: Longitudinal Bunch Pofile Measuements at TTF ) The time vaying fields in a tansvese mode cavity kick the font of a bunch up, and the back of the bunch don. ) A betaton phase advance of π late, the bunch adiates in an undulato 3) The vetical photon angles ae coelated ith the souce point 4) A slit, selecting only a shot ange of vetical angles, selects photons fom a small ange of souce points along the bunch. 5) A second cab cavity, a betaton phase advance of p afte the fist, kicks the tail up and the font don, compensating the vetical oscilations. 6) The bunch is typically about ps long, selecting ps educes the intensity to appoimately %. Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

3 Shot Pulses in Rings Mico-bunching: Longitudinal Bunch Pofile Measuements at TTF ) Instead of a slit, one can use an -ay bunch compesso. It poduces a time of flight that depends on the vetical angle to eliminate the coelation beteen vetical angle and souce point location. X-ay compession in asymmetic-cut cystals ) Realistically: tansmits up to 5% of beam due to collimation and losses. Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

4 Optics : Whee is the vetical Dipole? HERA Tunnel Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

5 Optics : Real Quadupoles SLAC The coils sho that this is an upight quadupole not a otated o ske quadupole. PETRA Tunnel Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

6 Optics 3: Real Setupoles ESRF Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

7 B Finge Fields and Main Fields 443 443 Main field Finge field Only the finge field egion has tems ith ψ z Main fields in acceleato physics: z ψ Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

8 Comple Potentials + iy, iy + + y, + z y i ( i + ) i( ( ) ) + z 4 + z ψ Im{ ψ Im{ λ, λ a, λ 4a ( z) λ λ ( ) } Im{ a ( ) ( λ + ) λ( ) λ λ, λ } λ } Iteation equation: a λ fo λ, a Ψ The functions Ψ detemine the complete field inside a magnet. Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

9 Finge Fields and Main z ψ Fields Only the finge field egion has tems ith ψ z Main fields in acceleato physics: z ψ Im{ ψ Ψ } Nice ay to deive multipole fields ψ (, ϕ) Ψ Im{ e i ( ϕ ϑ ) } Relation beteen adial poe and azimuthal symmety! The inde descibes C Symmety aound the z-ais e z due to a sign change afte ϕ π 3 Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8 S N N S S N

3 ψ Ψ Im{ iy Ψ y B ψ Ψ } C Symmety Multipoles in Acceleatos : Dipoles - (+,-) in Ψ e y + (S,N) in B + - Equipotential y const. B dp dt q v B Dipole magnets ae used fo steeing the beams diection dϕ Bending adius: dp dt ρ ρ p qvb p qb dp p dϕ ρ dl dϕ vdt dp / p p qb Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

3 Multipoles in Acceleatos : Quadupoles ψ Ψ Im{( iy) } Ψ y B Ψ ψ y - + C Symmety + - - + + - y z In a quadupole paticles ae focused in one plane and defocused in the othe plane. Othe modes of stong focusing ae not possible. Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

3 3 3 y ψ Ψ3 Im{( iy) } Ψ3 ( y 3 y) B ψ Ψ3 3 y C 3 Symmety S N Nonlinea Optics - Setupoles S i) Setupole fields hadly influence the paticles close to the cente, hee one can lineaize in and y. B B Ψ N N 3 S ψ Ψ a + 3 3 y 3 y y + y 6Ψ3 ii) iii) y + In linea appoimation a by shifted setupole has a quadupole field. When depends on the enegy, one can build an enegy dependent quadupole. O( ) k 3 Ψ3 k k! Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8

33 '' + ( k + κ ) Second-Ode Dispesion Fist ode in, '' + ( k κ f f ( δ ) κδ + ) Fist ode in,, δ D'' δ + K Dδ D s ˆ κ ββˆ sin( ψ k + ) '' + ( κ f + f ( δ ) f ψˆ) dsˆ D'' + K D κ Second ode in,, δ f κ ( δ ' κδ + κ ) + k( δ κ) k f(, ', δ ) The enegy dependent dispeion: D D '' + K D s Geog.Hoffstaette@Conell.edu Class Phys 488/688 Conell Univesity 4//8 f ( D, D',) [ f ] ββˆ sin( ψ ψˆ) dsˆ