Tsing Hua University, Taiwan Solar Acoustic Holograms January 2008, Tucson Dean-Yi Chou.

Slides:



Advertisements
Similar presentations
Chapter 9 Light as a Wave.
Advertisements

Lesson 8 G3 Two Source Interference of Waves
Wave Behavior Another McGourty-Rideout Production.
The Wave Nature of Light Chapter 24. Properties of Light Properties of light include reflection, refraction, interference, diffraction, and dispersion.
Optics 1. 2 The electromagnetic spectrum Visible light make up only a small part of the entire spectrum of electromagnetic waves. Unlike sound waves and.
Chapter 24 Wave Optics.
Chapter 24 Wave Optics.
Chapter 24 Wave Optics.
UNIT 8 Light and Optics 1. Wednesday February 29 th 2 Light and Optics.
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.
Chapter 34 The Wave Nature of Light; Interference
IVA. Electromagnetic Waves and Optics
Interference Physics 202 Professor Lee Carkner Lecture 24.
Kirchhoff Approximation for multi-layer rough surface Noppasin Niamsuwan By ElectroScience Laboratory, Ohio State University.
Lecture 3 – Physical Optics
University Physics Midterm Exam Overview. 16. THE NATURE OF LIGHT Speed of light c = 3x10 8 m/s (in the vacuum) v = c/n (in the media) Formulas c = f.
Tsing Hua University, Taiwan Measurements of Acoustic Waves Scattered by Sunspots (Stanford, April 2011, LoHCo Workshop) Dean-Yi Chou Hui Zhao Ming-Hsu.
PHY 1371Dr. Jie Zou1 Chapter 37 Interference of Light Waves (Cont.)
EMLAB 1 Power Flow and PML Placement in FDTD. EMLAB 2 Lecture Outline Review Total Power by Integrating the Poynting Vector Total Power by Plane Wave.
Chapter 25: Interference and Diffraction
Diffraction vs. Interference
Chapter 37 Wave Optics. Wave optics is a study concerned with phenomena that cannot be adequately explained by geometric (ray) optics.  Sometimes called.
Copyright © 2009 Pearson Education, Inc. Chapter 32 Light: Reflection and Refraction.
Chapter 37 - Interference and Diffraction
The wave nature of light Interference Diffraction Polarization
Lecture 15 Interference Chp. 35 Topics –Interference from thin films –Due to the wave nature of light –Change in wavelength and phase change in a medium.
CHAPTER 37 : INTERFERENCE OF LIGHT WAVES
EXAMPLE Young’s double-slit experiment is performed with 589-nm light and a distance of 2.00 m between the slits and the screen. The tenth interference.
Random Media in Radio Astronomy Atmospherepath length ~ 6 Km Ionospherepath length ~100 Km Interstellar Plasma path length ~ pc (3 x Km)
ECE 299 Holography and Coherent Imaging Lecture 1 Gabor Holography David J. Brady Duke University Lecture 1: Gabor Holographywww.disp.duke.edu/~dbrady/courses/holography.
Thus, the image formed by lens 2 is located 30 cm to the left of lens 2. It is virtual (since i 2 < 0). 30 The magnification is m = (-i 1 /p 1 ) x (-i.
Diffraction is the bending of waves around obstacles or the edges of an opening. Huygen’s Principle - Every point on a wave front acts as a source of tiny.
Interference Patterns Constructive interference occurs at the center point The two waves travel the same distance –Therefore, they arrive in phase.
Interference Patterns Constructive interference occurs at the center point The two waves travel the same distance –Therefore, they arrive in phase.
S-110 A.What does the term Interference mean when applied to waves? B.Describe what you think would happened when light interferes constructively. C.Describe.
Interference in Thin Films, final
Ch 16 Interference. Diffraction is the bending of waves around obstacles or the edges of an opening. Huygen’s Principle - Every point on a wave front.
Wave superposition If two waves are in the same place at the same time they superpose. This means that their amplitudes add together vectorially Positively.
Review First Exam What have we learned? Any traveling sinusoidal wave may be described by y = y m sin(kx   t +  ) Light always reflects with an angle.
Optical Holography Martin Janda, Ivo Hanák Introduction Wave Optics Principles Optical holograms Optical Holography Martin Janda, Ivo Hanák Introduction.
Lecture Nine: Interference of Light Waves: I
The Wave Nature of Light
Lecture 24 Interference of Light.
Lecture 26-1 Lens Equation ( < 0 )  True for thin lens and paraxial rays.  magnification m = h’/h = - q/p.
台灣清華大學, 物理系 Helioseismology (II) Global and Local Helioseismology ( , 北京 ) 周定一 Dean-Yi Chou.
Local Helioseismology LPL/NSO Summer School June 11-15, 2007.
Chapter 15 Preview Objectives Combining Light Waves
Wave Optics Light interferes constructively and destructively just as mechanical waves do. However due to the shortness of the wave length (4-7 x
Interference of Light Waves
Chapter 24 Wave Optics. General Physics Review – optical elements.
Coupled wave theory By Daniel Marks September 10, 2009 ECE 299 Holography and Coherence Imaging Lecture 7 Duke University.
Searching for the Magnetic Fields at the Base of the Convection Zone Dean-Yi Chou Institute of Astronomy & Department of Physics Tsing Hua University,
Chapter 24 Wave Optics. Young’s Double Slit Experiment Thomas Young first demonstrated interference in light waves from two sources in Light is.
Lecture 26-1 Lens Equation ( < 0 )  True for thin lens and paraxial rays.  magnification m = h’/h = - q/p.
Computer Graphics: Illumination
Lecture 26-1 Lens Equation ( < 0 )  True for thin lens and paraxial rays.  magnification m = h’/h = - q/p.
The wave nature of light Interference Diffraction Polarization
Lens Equation ( < 0 ).
Interference of Light Waves
Wave superposition If two waves are in the same place at the same time they superpose. This means that their amplitudes add together vectorially Positively.
Wave superposition If two waves are in the same place at the same time they superpose. This means that their amplitudes add together vectorially Positively.
The Wave Nature of Light
Really Basic Optics Instrument Sample Sample Prep Instrument Out put
Diffraction and Thin Film Interference
Mirrors and Lenses Images can be formed by reflection from mirrors.
Interference Introduction to Optics Coherent source
Interference of Light Waves
Unit 2 Particles and Waves Interference
LoHCo Meeting – Tucson, December 13, 2005
Acoustic Holography Sean Douglass.
Presentation transcript:

Tsing Hua University, Taiwan Solar Acoustic Holograms January 2008, Tucson Dean-Yi Chou

Motivation Is it feasible to apply the principle of optical holography to a system of solar acoustic waves and active regions?

Contents Principle of optical holography. Concept of acoustic holography of active regions. Construct 3-D wave fields of the magnetic region from the acoustic hologram. Set up a simplified model to compute acoustic holograms of magnetic regions. 1. analogies and differences between two 2. difficulties Challenges and prospects.

Hologram(interference pattern) (time average)

Construction of Waves hologram diffraction field (Gabor’s in-line holgram)

Acoustic waves on the Sun

solar surface interference pattern Solar Acoustic Waves + Active Region (acoustic power map) perturbed region

Optical HolographySolar Acoustic Holography reference wave object hologram p-mode wave magnetic region acoutsic power map Analogies (coming from below) (near the surface) (on the surface)

Questions: 1. Can we detect the inference pattern (hologram) due to a magnetic region on the surface? 2. Can we use the observed hologram to construct the 3-D image of the magnetic region?

Optical HolographySolar Acoustic Holography 1. monochromatic 5. far field approximation 4. single reference wave finite band width wavelength ~ dimension of object ~ distance to hologram * multiple incident waves Differences 2. no boundary trapped in cavities 3. straight ray path curved ray path

If the width of power spectrum of a wave field is, the cohernt time of waves is coherent time of waves : central frequency : period of central frequency example 3.3 mHz 0.2 mHz (FWHM = 0.47 mHz) 2.6

solar surface trapped in cavities curved ray path multiple incident waves 2. Waves are approximately vertical near the surface 1. Refracted waves from the lower turning point are ignored. s a λ ~ a ~ s

Multiple Incident Waves If incident waves are, total waves are Intensity of hologram cross terms If different waves are uncorrelated, the contribution from cross terms is small. Total interference is the sum of interference of individual wave. interference term Summation of interferences of different waves reduces the visibility of fringes.

1. Set up a simplified model for scattering of acoustic waves by a magnetic region. 2. Solve for the scattered waves. 3. Compute the interference pattern (hologram) between incident wave and scattered wave. 4. Study the influence of various parameters on the hologram. 5. Compute the constructed wave field by illuminating the hologram with a reference wave. Model Study

Assume unperturbed medium is uniform, and the wave equation is Assume the interaction between waves and magnetic regions is described by sound-speed perturbations: time independent Wave equation becomes Source of scattering Wave Equation

Solution of Scattered Wave scattered wave with Green’s function and Born approximation wave equation total solution expressed in terms of Fourier components

Hologram Intensity of the hologram is the time average of interference Interference term Need a model for spatial dependence of

A Simplified Model for assumptions: 1. Consider only one upward wave mode and its reflected wave at the surface. 2. Assume the free-end boundary at the surface. interference term normalized interference term (related to fringe visibility) 3. Simple dispersion relation:

Normalized Interference Term (fringe visibility) Effects of parameters on holograms 1. coherent time of incident waves 3. size of the perturbed region 4. depth of the perturbed region 2. wavelength 5. angle of incidence

Effects of Coherent Time of Incident Waves Setup of incident wave 3. Modes with a Gaussian power spectrum centered at 3.3 mHz, with different widths. 1. Waves propagate vertically: 2. Dispersion relation: 4. coherent time Perturbed region 1. Uniform cylinder with 2. diameter = 9.6 Mm, vertical extent = 4.8 Mm, depth = 12 Mm 3.3 mHz,14.7 Mm (l=300),48.5 km/s

Effects of Coherent Time 0.2 mHz (FWHM = 0.47 mHz) line width

Effects of Wavelength 3.3 mHz,0.2 mHz uniform cylinder with diameter = 9.6 Mm, vertical extent = 4.8 Mm, depth = 12 Mm wavelength

Effects of Angle of Incidence At 5Mm depth, the angle of incidence is about for at 3.3 mHz. for at 3.3 mHz. Waves with different phase velocities have different angles of incience. For example:

Effects of Angle of Incidence (cont.) 3.3 mHz,0.2 mHz, uniform cylinder with diamter = 9.6 Mm, vertical extent = 4.8 Mm, depth = 12 Mm 14.7 Mm (l=300) incident angle

Construction of Wave Fields from Holograms Illuminate the hologram by a vertically-propagating monochromatic wave. hologram on the surface

Advantages of digital holograms DC signal 2. Disentangling wave fields of virtual and real images. 1. DC signals are removed to enhance the interference pattern.

hologram on the surface Diffraction waves are computed by the Kirchhoff intergral replaced by

Constructed wave field 205 Mm 30 Mm Incident angle = 0 Mm depth = 30 Mm

Constructed wave field Incident angle = 0 deg. Depth = 30 Mm Incident angle = 0 deg. Depth = 12 Mm

Constructed wave field Incident angle = 0 deg. Depth = 30 Mm Incident angle = 10 deg. Depth = 30 Mm

Effects of Multiple Incident Waves 1. Weaken holograms 2. Distort and weaken constructed wave fields

The maximum occurs at. 1. Signals of holograms are weak. Challenges in detecting interference fringes 2. Interference fringes are contaminated by suppression of acoustic power in magnetic region. Fluctuation of 1000 MDI Dopplergrams is about 10%. 1% for the 2nd and 3rd fringes if Remove suppression by an empirical relation of power vs. field strength. Search for interference fringes outside magnetic regions. 3. Find an optimal filter to detect interference fringes.

power map before correctionpower map after correction magnetic fieldPower vs. B field 1024 MDI FD images

phase-velocity-filtered power map magnetic fieldpower map 1024 MDI FD images phase-velocity-filtered power map (3.3mHz/300)(3.3mHz/400)

power map before correctionpower map after correction magnetic fieldPower vs. B field 512 MDI HR images

Challenges in Constructed 3D Wave Fields 2. Is there a better way to construct 3D wave fields? 1.How to disentangle wave fields of virtual and real images and obtain the 3D structure of the magnetic region?

Improvement in computing interference fringes 1. A better model to compute scattered waves. 2. Study of simulation data interaction between waves and B fields more realistic dispersion relation Prospects Better Data Hinode & HMI