Quantification of Chromatic Aberration In the Laser-Heated Diamond Anvil Cell Emily England, Wes Clary, Daniel Reaman, Wendy Panero School of Earth Sciences,

Slides:



Advertisements
Similar presentations
Waves (in general) sine waves are nice
Advertisements

Wave Nature of Light  Refraction  Interference  Young’s double slit experiment  Diffraction  Single slit diffraction  Diffraction grating.
Copyright © 2009 Pearson Education, Inc. Chapter 35 Diffraction and Polarization.
Interference and Diffraction
The Wave Nature of Light
PHYS 1442 – Section 004 Lecture #21 Wednesday April 9, 2014 Dr. Andrew Brandt Ch 24 Wave Nature of Light Diffraction by a Single Slit or Disk Diffraction.
Foundations of Physics
Chapter 15 Pretest Light and Refraction
Frequency and Wavelength How are frequency, wavelength, and speed related for electromagnetic radiation in empty space? –speed = frequency x wavelength,
OPTICS. I. IMAGES A. Definition- An image is formed where light rays originating from the same point on an object intersect on a surface or appear to.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 28 Physics, 4 th Edition James S. Walker.
Chapter2: Light and EM Spectrum 18.1 The Electromagnetic Spectrum 18.2 Interference, Diffraction, and Polarization 18.3 Special Relativity Professor Mohammad.
Chapter 25: Interference and Diffraction
This Set of Slides This set of slides deals with telescopes. Units covered: 26, 27, 28, 29, and 30.
WAVES MEDIUM VIBRATES PERPENDICULARLY TO THE WAVE DIRECTION IF f IS THE WAVE FREQUENCE AND λ IS THE WAVELEGTH THEN c, THE WAVE VELOCITY, IS GIVEN BY: c.
Chapter 17 Optics 17.1 Reflection and Refraction
Microscope.
LIGHT. Reflection of light When light is reflected off of a mirror it forms an image. Mirror Incident ray Reflected ray Normal.
5 Components Common to All Optical Spectrometers Source Transparent Sample Holder Wavelength Selector Radiation Detector Signal Processor and Readout.
Chapter 23 Mirrors and Lenses.
Fundamental Physics II PETROVIETNAM UNIVERSITY FUNDAMENTAL SCIENCES DEPARTMENT Vungtau, 2013 Pham Hong Quang
Copyright © 2008 Pearson Education Inc., publishing as Pearson Addison-Wesley Reflected image Draw one ray from the object that enters the eye after reflecting.
Refraction is the change of direction of a light wave caused by a change in speed as the wave crosses a boundary between materials.
Optics 2: REFRACTION & LENSES. REFRACTION Refraction: is the bending of waves because of the change of speed of a wave when it passes from one medium.
Quiz Not graded 2. Color and Temperature Why does an opaque and dense object (such as metal) first glow white before it glows blue when it is heated?
Chapter 24 Wave Optics. General Physics Review – waves T=1/f period, frequency T=1/f period, frequency v = f velocity, wavelength v = f velocity, wavelength.
1. Waves and Particles 2. Interference of Waves
Simple Double Beam Spectrometer
Simple Double Beam Spectrometer
Optical Phenomenal Chapter 14 section 3. Objectives  Predict whether light will be refracted or undergo total internal reflection.  Recognize atmospheric.
1. How is the index of refraction calculated? How is light refracted as it speeds up? How is light refracted as it slows down? Index of refraction = speed.
Light Wave Interference In chapter 14 we discussed interference between mechanical waves. We found that waves only interfere if they are moving in the.
PowerPoint Lectures to accompany Physical Science, 7e Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter.
Unit 12: Part 1 Physical Optics: The Wave Nature of Light.
Physics 203/204 6: Diffraction and Polarization Single Slit Diffraction Diffraction Grating Diffraction by Crystals Polarization of Light Waves.
Electromagnetic Waves
© Houghton Mifflin Harcourt Publishing Company Preview Objectives Refraction of Light The Law of Refraction Sample Problem Chapter 14 Section 1 Refraction.
The Nature of Light. Light Can Act Like Waves or In 1801 Thomas Young an English scientist did an experiment. –Double slit experiment Passed a beam of.
Chapter 24 Wave Optics Conceptual Quiz Questions.
Physics 1202: Lecture 26 Today’s Agenda Announcements: –Midterm 2: Friday Nov. 6… –Chap. 18, 19, 20, and 21 No HW for this week (midterm)No HW for this.
Conditions for Interference
Refraction P 7.2 LIGHT TELESCOPES AND IMAGES. You should understand that the wave speed will change if a wave moves from one medium into another a change.
Copyright © by Holt, Rinehart and Winston. All rights reserved. ResourcesChapter menu Refraction Chapter 14 Table of Contents Section 1 Refraction Section.
Chapter 24 The Wave Nature of Light
Chapter 14 Preview Objectives Refraction of Light
Laser heating in the diamond anvil cell. mineral properties at high P,T constrain phases, temperature, and composition of earth & planets’ interiors understand.
Stellar Properties. A. Optical Telescopes a.Three properties that aid astronomers: i. LIGHT GATHERING POWER - ability to intercept more light, producing.
Copyright © by Holt, Rinehart and Winston. All rights reserved. ResourcesChapter menu Section 1 Refraction Chapter 14 Refraction of Light The speed of.
Refraction of Light Chapter 18, Section 1. Refraction  When light encounters a transparent or translucent medium, some light is reflected from the surface.
Chapter 24 Wave Optics. Young’s Double Slit Experiment Thomas Young first demonstrated interference in light waves from two sources in Light is.
Young's double-slit experiment
Light and Optics  The Electromagnetic Spectrum  Interference, Diffraction, and Polarization Wave Properties of Light.
Refraction & Lenses. Refraction of Light When a ray of light traveling through a transparent medium encounters a boundary leading into another transparent.
 Electromagnetic Radiation › Gamma rays, X-rays, UV light, visible light, infrared radiation, microwaves, and radio waves › All energy travels through.
Phys102 Lecture 26, 27, 28 Diffraction of Light Key Points Diffraction by a Single Slit Diffraction in the Double-Slit Experiment Limits of Resolution.
Light & Optics Physics I By Lynn Johnson.
Microscope.
Simple Double Beam Spectrometer
“Whether they ever find life there or not, I think Jupiter should be considered an enemy planet.” Jack Handy HW2 is due on Wednesday. How’s that going?
Chapter 35-Diffraction Chapter 35 opener. Parallel coherent light from a laser, which acts as nearly a point source, illuminates these shears. Instead.
Light Waves Interacting with Matter
PRISMS – one of the e.g. of optical instrumentation
Light Waves Interacting with Matter
QOD: What happens to the rays with a diverging lens?
Refraction Optical Phenomena.
Refraction Optical Phenomena.
Presentation transcript:

Quantification of Chromatic Aberration In the Laser-Heated Diamond Anvil Cell Emily England, Wes Clary, Daniel Reaman, Wendy Panero School of Earth Sciences, The Ohio State University Introduction Earth materials subjected to the high pressure and temperature conditions of planetary interiors display unique changes in crystal structure, melting temperature, and transport properties.Earth materials subjected to the high pressure and temperature conditions of planetary interiors display unique changes in crystal structure, melting temperature, and transport properties. The laser-heated diamond anvil cell (LHDAC) is a tool to make in situ measurements of material properties, specifically at pressures up to 1 Mbar (100 GPa) and temperatures from 1500 to 7000 K. Temperatures above 1500 K are measured by the spectroradiometry of the thermal emission that passes through the diamond anvil and is collected on a intensity-calibrated spectrometer and coupled-charged device (CCD).The laser-heated diamond anvil cell (LHDAC) is a tool to make in situ measurements of material properties, specifically at pressures up to 1 Mbar (100 GPa) and temperatures from 1500 to 7000 K. Temperatures above 1500 K are measured by the spectroradiometry of the thermal emission that passes through the diamond anvil and is collected on a intensity-calibrated spectrometer and coupled-charged device (CCD). The accuracy of the measured temperatures is not always reliable, due to optical dispersion of the diamond and lenses in the system. The size of the laser-heated spot on the sample is only about 20 micrometers. This small hot spot leads to large spatial variations in intensity as a function of wavelength. This variation requires focusing and magnification of light through the optical system with minimal chromatic aberrations.The accuracy of the measured temperatures is not always reliable, due to optical dispersion of the diamond and lenses in the system. The size of the laser-heated spot on the sample is only about 20 micrometers. This small hot spot leads to large spatial variations in intensity as a function of wavelength. This variation requires focusing and magnification of light through the optical system with minimal chromatic aberrations. X-ray diffraction (pressure, structure, density) The Laser Heated Diamond Anvil Cell (LHDAC) 2 cm Pressure = Force/Area Spectroradiometry (temperature) Heating laser 0.1 mm X-ray Methods To quantify the chromatic aberrations, we will use a high birefringence material to test each component (lenses, mirrors, beam splitters, etc.) of the laser system.To quantify the chromatic aberrations, we will use a high birefringence material to test each component (lenses, mirrors, beam splitters, etc.) of the laser system. The material we have chosen to measure the system’s chromatic aberration a thin section of olivine. This will provide a “color standard” to test how well the system focuses each wavelength of visible light ( nm).The material we have chosen to measure the system’s chromatic aberration a thin section of olivine. This will provide a “color standard” to test how well the system focuses each wavelength of visible light ( nm). Specifically, light will pass through the olivine between crossed-polarizers then through the diamond, then the rest of the system.Specifically, light will pass through the olivine between crossed-polarizers then through the diamond, then the rest of the system. Path of Light Through System Walter and Koga, 2004 Olivine as a Image and Spectrum Test The origin of chromatic aberration is the wavelength-dependant index of refraction, or dispersion, of refracting optical components, especially the diamond.The origin of chromatic aberration is the wavelength-dependant index of refraction, or dispersion, of refracting optical components, especially the diamond. Specifically, Birefringence is the effect that the refractive index which a light beam experiences in a non-isotropic medium depends on the polarization direction.Specifically, Birefringence is the effect that the refractive index which a light beam experiences in a non-isotropic medium depends on the polarization direction. Birefringence colors in thin materials Laser System Olivine Images This is a image of the olivine as focused on the spectrometer.  Image and spectrum of a 1 slit through the middle of the above image. The spectrometer grating is centered at 600nm. This disperses the light with red falling to the right and blue falling to the left..  Image and spectrum of a 11 mm slit through the middle of the above image. The spectrometer grating is centered at 600nm. This disperses the light with red falling to the right and blue falling to the left.. Olivine + Diamond Images This is an image of the olivine as viewed through the diamond and focused on the spectrometer.  Image and spectrum after spectrometer mirror was set to 600nm. Notice that wavelengths are not focused as well. Conclusions The refraction of the diamond (dispersion = 0.044) causes loss of both image and spectral resolution at the imaging spectrometer.The refraction of the diamond (dispersion = 0.044) causes loss of both image and spectral resolution at the imaging spectrometer. Further research is needed to quantify the magnitude of the problem and its effect on the measurement of temperatures and temperature measurements in the laser-heated diamond anvil cell.Further research is needed to quantify the magnitude of the problem and its effect on the measurement of temperatures and temperature measurements in the laser-heated diamond anvil cell. Likely solutions include duplication of the measurement to use images of the total intensity paired with spectra of the central portion of the hotspot (See Clary et al)Likely solutions include duplication of the measurement to use images of the total intensity paired with spectra of the central portion of the hotspot (See Clary et al) References Benedetti, L. R., N. Guignot, and D. L. Farber, Achieving accuracy in spectroradiometric measurements of temperature in the laser-heated diamond anvil cell: Diamond is an optical component. Journal of Applied Physics, 101, , 2007.Benedetti, L. R., N. Guignot, and D. L. Farber, Achieving accuracy in spectroradiometric measurements of temperature in the laser-heated diamond anvil cell: Diamond is an optical component. Journal of Applied Physics, 101, , Walter, M. J. and K. T. Koga, The effects of chromatic dispersion on temperature measurement in the laser-heated diamond anvil cell, Phys. Earth. Planet Int., , , 2004.Walter, M. J. and K. T. Koga, The effects of chromatic dispersion on temperature measurement in the laser-heated diamond anvil cell, Phys. Earth. Planet Int., , , mm Diamond and Dispersion The index of refraction of diamond is higher for blue light than red, causing blue light to be refracted at a greater angle as it travels through the diamond. Diamond is a high-dispersion material and in the LHDAC, the thermal emission must refract through the diamond anvil in order to reach the spectrometer. Benedetti et al., 2007 Dispersion of Light Through System Walter and Koga, 2004 The effect of dispersion is to focus blue more tightly than red. Therefore, an image that appears in focus in one color of light will be out of focus in another color. This leads to a loss of both spectral and image resolution. 2.5 mm The birefringence color seen depends on the thickness of the material (horizontal lines) and the birefringence (diagonal lines) Olivine has a birefringence of about , labeled forsterite (Mg 2 SiO 4 ) and fayalite (Fe 2 SiO 4 ) at right. The observed color is a function of both composition and orientation of the grain with respect to the polarizer. Our specific olivine sample has an unusual color variation with position, varying from blue to red with a sharp boundary between, providing a spatially dependent color signal. The light passes from the source (“object plane”) through an objective and focusing lens. The light is then focused on the image plane of the imaging spectrometer where a thin slit of light (11 mm) is dispersed with a 600 groove per inch spectrometer in a m spectrometer. Olivine Thin Section Olivine in plane light Olivine in crossed polarized light. The image and spectral test was performed along the black line. Image of olivine through TV camera position wavelength blue light red light wavelength position blue light red light 2.5 mm