Lecture 4.

Slides:



Advertisements
Similar presentations
Overview of SPM p <0.05 Statistical parametric map (SPM)
Advertisements

So far Geometrical Optics – Reflection and refraction from planar and spherical interfaces –Imaging condition in the paraxial approximation –Apertures.
BIOP – Center for Biomedical Optics and New Laser Systems Light scattering from a single particle Peter E. Andersen Optics and Fluid Dynamics Dept. Risø.
Ray theory and scattering theory Ray concept is simple: energy travels between sources and receivers only along a “pencil-thin” path (perpendicular to.
Dr. Daniel F.V. James MS B283, PO Box 1663, Los Alamos NM Invited Correlation-induced spectral (and other) changes Daniel F. V. James, Los Alamos.
Neutron Scattering Theory For Bio-Physicists Hem Moktan Department of Phycis Oklahoma State University.
Lesson 3 METO 621. Basic state variables and the Radiative Transfer Equation In this course we are mostly concerned with the flow of radiative energy.
Evan Walsh Mentors: Ivan Bazarov and David Sagan August 13, 2010.
Statistical Properties of Wave Chaotic Scattering and Impedance Matrices Collaborators: Xing Zheng, Ed Ott, ExperimentsSameer Hemmady, Steve Anlage, Supported.
Wave Optics. Wave Optics wave fronts (surfaces of constant action) are orthogonal to rays (a) spherical wave, (b) plane wave (c) dipole wave, (d) dipole.
The Klein Gordon equation (1926) Scalar field (J=0) :
Lecture 1 Review of Wave optics Today Introduction to this course Light waves in homogeneous medium Monochromatic Waves in inhomogeneous medium.
LESSON 4 METO 621. The extinction law Consider a small element of an absorbing medium, ds, within the total medium s.
Space-time analogy True for all pulse/beam shapes Paraxial approximation (use of Fourier transforms) Gaussian beams (q parameters and matrices) Geometric.
Wireless Communication Arjav A. Bavarva Dept. of Electronics and Communication.
Anharmonic Oscillator Derivation of Second Order Susceptibilities
K L University By G.SUNITA DEPARTMENT OF PHYSICS.
Microwave polarization plasma diagnostic Head of group: Prof. dr hab. Yu. Kravtsov, Institute of Physics, Maritime University of Szczecin Members of group:
Wave Optics. What is Light? Light is a name for a range of electromagnetic radiation that can be detected by the human eye. What is electromagnetic radiation?
Physics 452 Quantum mechanics II Winter 2011 Karine Chesnel.
3.7 Diffraction allows RF signals to propagate to obstructed (shadowed) regions - over the horizon (around curved surface of earth) - behind obstructions.
Nanostructures Research Group CENTER FOR SOLID STATE ELECTRONICS RESEARCH Time-Dependent Perturbation Theory David K. Ferry and Dragica Vasileska Arizona.
Scattering by particles
Focusing of Light in Axially Symmetric Systems within the Wave Optics Approximation Johannes Kofler Institute for Applied Physics Johannes Kepler University.
1 Topical Seminar on Frontier of Particle Physics 2004: QCD and Light Hadrons Lecture 1 Wei Zhu East China Normal University.
Introduction of Surface Scattering Modeling
ORE 654 Applications of Ocean Acoustics Lecture 6c Scattering 1 Bruce Howe Ocean and Resources Engineering School of Ocean and Earth Science and Technology.
Congresso del Dipartimento di Fisica Highlights in Physics –14 October 2005, Dipartimento di Fisica, Università di Milano An application of the.
3D scattering of electrons from nuclei
Physics 452 Quantum mechanics II Winter 2012 Karine Chesnel.
Complex geometrical optics of Kerr type nonlinear media Paweł Berczyński and Yury A. Kravtsov 1) Institute of Physics, West Pomeranian University of Technology,
Methods for describing the field of ionospheric waves and spatial signal processing in the diagnosis of inhomogeneous ionosphere Mikhail V. Tinin Irkutsk.
§9.6 High-Frequency Modulation Considerations Lecture 16 In practice, the modulation signal is often at very high frequencies and may occupy a large bandwidth,
Introduction to Time dependent Time-independent methods: Kap. 7-lect2 Methods to obtain an approximate eigen energy, E and wave function: perturbation.
Particle Detectors for Colliders Robert S. Orr University of Toronto.
Lecture 3. Full statistical description of the system of N particles is given by the many particle distribution function: in the phase space of 6N dimensions.
Physics 842, February 2006 Bogdan Popescu Presentation based on “Introduction to Elementary Particles” by David Griffiths WEAK INTERACTION (1)
Synchrotron radiation: generation, coherence properties and applications for beam diagnostics Gianluca Geloni European XFEL GmbH.
Instability of optical speckle patterns in cold atomic gases ? S.E. Skipetrov CNRS/Grenoble (Part of this.
Announcements Exam 3 starts Thur noon, and continues through Mon close, in the Testing Center. It will include both conceptual questions and homework style.
Energy loss in abelian medium M. Kirakosyan, Lebedev Institute A. Leonidov, Lebedev Institute and ITEP Quarks
Introduction to Scattering Theory
Polarization of final electrons/positrons during multiple Compton
Theory of Scattering Lecture 2.
Radio Coverage Prediction in Picocell Indoor Networks
PHYS 408 Applied Optics (Lecture 16)
PHYS 408 Applied Optics (Lecture 21)
Nuclear reaction and scattering theory
PHYS 408 Applied Optics (Lecture 15)
Introduction to Diffraction Tomography
X Ray Diffraction © D Hoult 2009.
Diffraction LL2 section 59.
Chap-2: Waves and Sound Wave is a traveling disturbance.
LECTURE 3.
Lecture 5.
Chapter V Interacting Fields Lecture 7 Books Recommended:
Wave-Equation Migration Research at Los Alamos National Laboratory
Fraunhofer Diffraction
PHY 752 Solid State Physics
Summary of Lecture 18 导波条件 图解法求波导模式 边界条件 波导中模式耦合的微扰理论
Observing screen is quite close to aperture
. y y’ A B a a’ = C D OPTICAL SYSTEM GEOMETRICAL OPTICS
Scattering Theory: Revised and corrected
Scalar theory of diffraction
Scalar theory of diffraction
Scalar theory of diffraction
PHY 752 Solid State Physics
ECE 6341 Spring 2016 Prof. David R. Jackson ECE Dept. Notes 29.
SPACE TIME Fourier transform in time Fourier transform in space.
X-Ray Diffraction Path Length Phase Difference
Presentation transcript:

Lecture 4

statistical description

stochastic equation is a random function

Parabolic (paraxial) approximation < > < > Small Perturbations; Local Perturbations; Smooth Perturbations; Path Integral Feynman diagrams Fokker-Plank Equation Random Matrix Theory Supersymmetry Parabolic (paraxial) approximation

propagator

< > < > < > < > < >

1 2 3

single scattering (first Born) approximation

random function < > < >

in the far zone

far zone

resonant Bragg scattering

V energy flux density Differential SCS

Total SCS

INVERSE PROBLEM

energy conservation

energy conservation ?

Extinction Length energy conservation !

small perturbation, weak total scattering (Energy of the scattered field) (Energy of the incident field)

smooth perturbations is not necessarily small new small parameter

Parabolic Approximation

Parabolic Equation

forward scattering backscattering

small angle of scattering

Geometrical Optics

eikonal amplitude

Phase fluctuations

Amplitude fluctuations

Multiple scattering! Compare to the result of the first Born approximation (single scattering) Gaussian random function

Transverse Ray Deflection Optical Magnus effect Transverse Ray Deflection POLARIZATION helicity

there is neither no polarization in the equations of rays helicity

Transverse Ray Deflection linear polarization

Limits of validity of GO approximation rays, no diffraction

Multiple scattering

<….……………………………… >

odd even Gaussian