LOW COST HYPERSPECTRAL

Slides:



Advertisements
Similar presentations
Plane wave reflection and transmission
Advertisements

IV. Optics Nature of light. Spectrum of electromagnetic waves.
Note on Fresnel transmission coefficient: Consider n1>n2  t>1 We still have conservation of Energy! Fresnel Coefficients:
Module 1-1 Continued Nature and Properties of Light.
Spectral Resolution and Spectrometers
Spectral Resolution and Spectrometers A Brief Guide to Understanding and Obtaining the Proper Resolution of the 785 Raman System.
Wavelike Properties of Electromagnetic Radiation 1.Wave parameters 2.Refraction a.Index of refraction Snell’s Law b. Prism monochrometers 3.Diffraction.
Lecture 33 Review for Exam 4 Interference, Diffraction Reflection, Refraction.
Diffraction Applications Physics 202 Professor Lee Carkner Lecture 28.
Hyperspectral Imagery
Part IV: Optical Spectroscopy of Solids
5/1/06 Fiber Optics (continued) CD’s & DVD’s Poster Session: 2 – 5 pm Show up between 1:30 and 2 (if possible) to set up Schedule Reviews HW #8 due Wed.
Interference and Diffraction
Diffraction Applications Physics 202 Professor Lee Carkner Lecture 26.
Fiber-Optic Communications James N. Downing. Chapter 2 Principles of Optics.
Overlapping Orders Douglas A. Skoog and James J. Leary, Principles of Instrumental Analysis, Saunders College Publishing, Fort Worth, d(sin  + sin.
PHY 1371Dr. Jie Zou1 Chapter 38 Diffraction and Polarization (Cont.)
IV. Optics Nature of light. Spectrum of electromagnetic waves.
Diffraction Applications Physics 202 Professor Lee Carkner Lecture 28.
Refraction Physics Department, New York City College of Technology.
Refractive index Sections 36, 37 and 38. Refraction: When a wave changes direction as it passes from one medium to another.
Document Title/Description1 Our prism and Grating Spectrometer
Diffraction vs. Interference
1 The University Centre in Svalbard (UNIS), N-9171 Longyearbyen, Norway 2 Magnetosphere Ionosphere Research Lab, University of New Hampshire, USA 3 Keo.
Grazing-incidence design and others L. Poletto Istituto Nazionale per la Fisica della Materia (INFM) Department of Electronics and Informatics - Padova.
Refraction, Lenses, & Sight. Refraction The change in direction of a wave as is crosses the boundary between two media in which the wave travels at different.
Astronomical Instrumentation Often, astronomers use additional optics between the telescope optics and their detectors. This is called the instrumentation.
Rayleigh and Mie Scattering
The Refraction of Light: Lenses and Optical Instruments.
Mirrors & prisms MIT 2.71/ /12/01 wk2-b-1 Last time: optical elements, – Pinhole camera – Lenses Basic properties of spherical surfaces Ray tracing.
Principal maxima become sharper Increases the contrast between the principal maxima and the subsidiary maxima GRATINGS: Why Add More Slits?
Chapter 13 The Characteristics of light. Objectives Identify the components of the electromagnetic spectrum. Calculate the frequency or wavelength of.
Astronomical Spectroscopy Notes from Richard Gray, Appalachian State, and D. J. Schroeder 1974 in “Methods of Experimental Physics, Vol. 12-Part A Optical.
The Hong Kong Polytechnic University Optics 2----by Dr.H.Huang, Department of Applied Physics1 Diffraction Introduction: Diffraction is often distinguished.
Ch Refraction Definition: Refraction Change in speed of light as it moves from one medium to another. Can cause bending of the light at the interface.
The incoming wave travels at 5ms -1 and has a wavelength of 4m. The wave changes its speed once it moves onto a shallower region and as the result its.
Sight and Waves Part 2 Problem Solving Mr. Klapholz Shaker Heights High School.
Reflection and Refraction Chapter 17. Law of Reflection θiθi θrθr θ i angle of incidence θ i angle of reflection.
Refraction Chapter 15. Refraction Refraction: The bending of light as it travels from one medium to another Refraction occurs when light’s velocity changes.
Sensitivity Calibration of Narrow Field of View Optical Instruments F. Sigernes 1, T. Svenøe 2, J. Holmes 1, M. Dyrland 1, D.A. Lorentzen 1, J. Moen 3,
Refraction of Light When can light “bend”?.
NASA’s Coastal and Ocean Airborne Science Testbed (COAST) L. Guild 1 *, J. Dungan 1, M. Edwards 1, P. Russell 1, S. Hooker 2, J. Myers 3, J. Morrow 4,
AP Physics 2 Unit 7 Refraction and Physical Optics.
Final Exam Lectures EM Waves and Optics. Electromagnetic Spectrum.
Chapter 26 The Refraction of Light: Lenses and Optical Instruments.
Date of download: 6/1/2016 Copyright © 2016 SPIE. All rights reserved. Spatial (angular) resolution versus field angle for design with toroidal grating.
Light Reflection and Refraction. Reflection Law of Reflection.
Date of download: 6/24/2016 Copyright © 2016 SPIE. All rights reserved. Schematic diagram of rectangle diffraction phase grating with depth h, period Λ,
Sept 16, 2005Ast 920 Meeting 21 Astronomy 920 Commissioning of the Prime Focus Imaging Spectrograph Meeting 2 Intro; VPH Grating Spectroscopy Ken Nordsieck.
The Critical Angle and Total Internal Reflection.
Diffraction Gratings.
IV. Optics Nature of light. Spectrum of electromagnetic waves.
Hyperspectral Sensing – Imaging Spectroscopy
AIRS (Atmospheric Infrared Sounder) Instrument Characteristics
IV. Optics Nature of light. Spectrum of electromagnetic waves.
Reflection and Refraction
Physics 202 Lecture 9 Geometric Optics.
Light, Color, and Polarization
BASIC HYPER SPECTRAL IMAGING
Reflection and Refraction (Snell’s Law).
Instrument Considerations
BASIC HYPER SPECTRAL IMAGING
Behavior of Light.
BASIC HYPER SPECTRAL IMAGING
The scattering centre becomes a secondary source of radiation
Surface Waves.
Wave reflection and refraction
BASIC HYPER SPECTRAL IMAGING
Chapter 14 Refraction.
Chapter 33 Electromagnetic Waves
Presentation transcript:

LOW COST HYPERSPECTRAL IMAGING AT UNIS F. Sigernes The University Centre on Svalbard, Norway

SCENARIO = REMOTE SENSING SVALSAT is well established. All polar satellites in field of view. Longyearbyen airport. Local airborne carriers. AGF-207, AGF-331 & AGF-218 Logistics CryoWing UAV w/ NORUT IT   = REMOTE SENSING

PRINCIPLE

KEY OPTICAL ELEMENT   The grating equation is modified by using Snell’s law where m is the spectral order, l is the wavelength, a the groove spacing, a the incident angle and b the diffracted angle. Wavelength l [nm] Refractive index n Diffracted angle b [deg.] BP [ nm] Linear dispersion dl/dx [nm/mm] 300 1.61829 38.9872 0.63 37.9174 400 1.58942 33.6908 0.74 48.0392 500 1.57606 29.2111 0.80 53.9186 600 1.56880 25.1126 0.82 57.7198 700 1.56442 21.2360 0.83 60.3967 800 1.56158 17.5051 0.84 62.3734 900 1.55963 13.8757 0.85 63.8542

CALIBRATION-CALIBRATION-CALIBRATION  

NEW LOW COST INSTRUMENT   NEW LOW COST INSTRUMENT

SETUP DORNIER 228 LUFTTRANSPORT SLIDING DOOR SIDE VIEW 30 DEG. V = 200 KM / HR Z = 3000 M

REGULAR STUFF!  

AIRBORNE APPLICATIONS  

AIRBORNE APPLICATIONS

AIRBORNE APPLICATIONS   AIRBORNE APPLICATIONS

AIRBORNE APPLICATIONS   AIRBORNE APPLICATIONS

AIRBORNE APPLICATIONS  

SMALL APPLICATIONS

SMALLER APPLICATIONS

REALY SMALL APPLICATIONS   REALY SMALL APPLICATIONS

REALY SMALL APPLICATIONS   REALY SMALL APPLICATIONS