Lecture 20 – review Labs: questions Next Wed – Final: 18 March 10:30-12:20 Thursday, 12 March.

Slides:



Advertisements
Similar presentations
Electro-magnetic radiation
Advertisements

Radiometric Corrections
Electromagnetic Radiation Electromagnetic Spectrum Radiation Laws Atmospheric Absorption Radiation Terminology.
Thermal Infrared Remote Sensing Radiant versus Kinetic temperature Blackbody radiation Atmospheric effect Principle of energy conservation Radiation from.
ESS 421 – Introduction to Geological Remote Sensing Prof: Alan Gillespie (JHN 343) Office hours: Wed - Fri or by arrangement TA: Iryna.
Landsat-based thermal change of Nisyros Island (volcanic)
1. 2 Definition 1 – Remote sensing is the acquiring of information about an object or scene without touching it through using electromagnetic energy a.
Electromagnetic radiation : Interaction with matter and atmosphere
Lesson 7: Remote Sensing Dr Andrew Ketsdever MAE 5595.
Lecture 12: Image Processing Friday 11 February 2011 Last lecture: Earth-orbiting satellites Reading Ch
Lecture 13: Spectral Mixture Analysis Wednesday 16 February 2011 Reading Ch 7.7 – 7.12 Smith et al. Vegetation in deserts (class website)
Lecture 4: The spectrum, color theory and absorption and photogrammetry Friday, 14 January 1 Reading: Ch 2.3 – photography basics.
Weighting Functions for Microwave and Infra-Red Satellite Nadir Sounding Remote Sensing I Lecture 7 Summer 2006.
ESS st half topics covered in class, reading, and labs Images and maps - (x,y,z,,t) Temporal data - Time-lapse movies Spatial data - Photos and.
Lecture 5: Radiative transfer theory where light comes from and how it gets to where it’s going Wednesday, 19 January 2010 Ch 1.2 review, 1.3, 1.4
Energy interactions in the atmosphere
Class 10: Earth-Orbiting Satellites And Review Thursday 5 February Reading: LKC p Last lecture: Spectroscopy, mineral spectra.
Lecture 2 Photographs and digital mages Friday, 7 January 2011 Reading assignment: Ch 1.5 data acquisition & interpretation Ch 2.1, 2.5 digital imaging.
Lecture 14: Classification Thursday 18 February 2010 Reading: Ch – 7.19 Last lecture: Spectral Mixture Analysis.
Lecture 4: The spectrum, color theory and absorption and photogrammetry Thursday, 14 January Ch 2.3 (color film)
Lecture 12: Image Processing Thursday 12 February Last lecture: Earth-orbiting satellites Reading, LKC p
Lecture 14: Classification Thursday 19 February Reading: “Estimating Sub-pixel Surface Roughness Using Remotely Sensed Stereoscopic Data” pdf preprint.
Lecture 13: Searching for planets orbiting other stars I: Properties of Light 1.How could we study distant habitats remotely ? 2.The nature of light -
Remote Sensing in Geology, Siegal & Gillespie (class website)
Radiation: WHY CARE ??? the ultimate energy source, driver for the general circulation usefully applied in remote sensing (more and more)
Electromagnetic Radiation. Is light a wave or a particle? Yes It’s both, and neither At atomic scales, we have no exact analogs for phenomena For some.
1 Interaction Between Radiation and the Material Prof. Arnon Karnieli The Remote Sensing Laboratory Jacob Blaustein Institute for Desert Research Ben-Gurion.
Predicting Engine Exhaust Plume Spectral Radiance & Transmittance
Remote Sensing Energy Interactions with Earth Systems.
Spectral Characteristics
刘瑶.  Introduction  Method  Experiment results  Summary & future work.
Welcome Back Write down the 4 layers of the atmosphere (in order) and 1 fact about each.
 Introduction to Remote Sensing Example Applications and Principles  Exploring Images with MultiSpec User Interface and Band Combinations  Questions…
Digital Imaging and Remote Sensing Laboratory Spectral Signatures.
EG2234: Earth Observation Interactions - Land Dr Mark Cresswell.
Remote Sensing Classification Accuracy
Digital Imaging and Remote Sensing Laboratory Thermal Infrared Spectral Analysis Thermal absorption/emissivity structure (3-20 µm) can be indicative of.
Topic 6. Without energy from the sun, conditions on Earth would be different. What is the energy that is radiated from the Sun? The energy that is radiated.
Lecture 5: Radiative transfer theory where light comes from and how it gets to where it’s going Tuesday, 19 January 2010 Ch 1.2 review, 1.3, 1.4
Remote Sensing in Geology. Lesson 1: Definition and scope of Remote Sensing Brief history Lesson 2: RS system Elements of the RS system Lesson 3: Resources.
Electromagnetic Radiation: Interactions in the Atmosphere.
Radiation (Ch 12 YAC) Thermal energy is emitted by matter as a result of vibrational and rotational motion of molecules, atoms and electrons. The energy.
Remote Sensing Waves transport energy. According to quantum theory, light may be considered not only as an electro-magnetic wave but also as a "stream"
Quick Review of Remote Sensing Basic Theory Paolo Antonelli SSEC University of Wisconsin-Madison Monteponi, September 2008.
Lecture 8: Volume Interactions Thursday, 28 January 2010 Ch 1.8 Major spectral features of minerals (p. xiii-xv), from Infrared.
Energy, heat, and absorption Scripps Classroom Connection
Remote sensing/digital image processing. Color Arithmetic red+green=yellow green+blue=cyan red+blue=magenta.
Remote Sensing Part 2 Atmospheric Interactions & Pre-processing.
Heat Transfer RADIATION HEAT TRANSFER FUNDAMENTALS.
Energy Flow Concept Image Sensor Energy Source
Class 12 Assessment of Classification Accuracy
Landsat-based thermal change of Nisyros Island (volcanic)
ESS st half topics covered in class, reading, and labs
Lecture 8: Volume Interactions
Lecture 9: Spectroscopy
Lecture 9: Spectroscopy
Radiation Thermal energy emitted by matter as a result of vibrational and rotational movements of molecules, atoms and electrons. The energy is transported.
Radiation in the Atmosphere
Tuesday, 20 January Lecture 5: Radiative transfer theory where light comes from and how it gets to where it’s going
Lecture 8: Volume Interactions
ESS 421 – Introduction to Geological Remote Sensing
Lecture 9: Spectroscopy
Lecture 20 – review Thursday, 11 March 2010 Labs: questions
Radiation Thermal energy emitted by matter as a result of vibrational and rotational movements of molecules, atoms and electrons. The energy is transported.
Class 10: Earth-orbiting satellites
Introduction and Basic Concepts
Lecture 8: Volume Interactions
Lecture 12: Image Processing
Lecture 9: Spectroscopy
Presentation transcript:

Lecture 20 – review Labs: questions Next Wed – Final: 18 March 10:30-12:20 Thursday, 12 March

- physical basis of remote sensing - spectra - radiative transfer - image processing - radar/lidar -thermal infrared - applications

What is remote sensing? Measurement from a distance Wide range of wavelengths Hazardous locales Images pixels DNs scanners, orbits image geometry, parallax resolution color vs. intensity and texture

The spectrum and wavelength regions Units of radiance, irradiance, spectral radiance Color mixing, RGB false color images Color is due to absorption: e -kz (Beer Law) Hue, saturation, intensity

Radiative transfer Sunlight, atmospheric absorption & scattering Rayleigh, Mie, Non-selective Reflection – 1 st surface (Fresnel’s Law), volume Planck function: -5 (exp(c/ T)-1)  Atmospheric windows DN = g·(  e ·r ·  i ·I toa ·cos(i)/  +  e · r·I s↓ /  + L s↑ ) + o r I cos(i)/  : Lambert’s law

When do you need atmospheric compensation? dark object subtraction Modtran model

Interaction of Energy and Matter Rotational absorption (gases) Electronic absorption Charge-Transfer Absorptions Vibrational absorption Spectra of common Earth-surface materials

Image processing algorithms radiometry geometry Spectral analysis Statistical analysis Modeling Algorithms: Ratioing Spectral mixture analysis max number of endmembers = n+1 shade NDVI

Classification – spectral similarity supervised vs. unsupervised maximum likelihood vs parallelipiped themes & land use validation confusion matrix

Confusion matrices Well-named. Also known as contingency tables or error matrices Here’s how they work… Training areas A B C D E F A B C D E F Classified data Col sums Row sums Grand sum All non diagonal elements are errors Row sums give “commission” errors Column sums give “omission” errors Overall accuracy is the diagonal sum over the grand total This is the assessment only for the training areas What do you do for the rest of the data? p 586, LKC 6 th

Crater counting – relative dating on the moon and Mars Forest remote sensing SMA in forest studies Shade endmember vs. canopy vs. topography What can Lidar do for forest characterization?

Layover Shadows Polarization Sensitivity to - dielectric - roughness Corner reflectors Interferometry

LiDAR

Thermal  ( ) T Planck’s Law: R =  ( ) c 1  -1 -5 [exp(c 2 -1 T -1 )-1] -1 Emissivity Blackbody radiation

What compositions can be determined in the TIR? Mostly vibrational resonance, not electronic processes therefore, relatively large molecules Silicate minerals (SiO 4 -4 ); quartz (SiO 2 ) Sulfates (SO 4 = ); sulfur dioxide (SO 2 ) Carbonates (CO 3 = ); carbon dioxide (CO 2 ) Ozone (O 3 ) Water (H 2 O) Organic molecules

Mauna Loa, Hawaii MASTER VNIR daytime ASTER TIR, daytime MTI TIR, nighttime