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Our atmosphere

Lecture 3 Remote Sensing in the Visible and Reflected IR Region of the EM spectrum - The Effects of the Atmosphere on EM Radiation February 9th 2009.

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Our atmosphere

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  1. Lecture 3 Remote Sensing in the Visible and Reflected IR Region of the EM spectrum - The Effects of the Atmosphereon EM RadiationFebruary 9th 2009

  2. SyllabusLecture/Hourly Exam Schedule and Assigned Readings (Subject to Change) Week Date Lecture Topic Reading Part I Remote Sensing Basics 1 26-Jan 1 Introduction to Remote Sensing Ch 1 28-Jan University Closed2 02-Feb 2 Principles of EM radiometry and basic EM Theory Ch 2 04-Feb Principles of EM radiometry and basic EM Theory II3 09-Feb3 Atmospheric Influences on EM Radiation 11-Feb 4 Photographic Systems/Image InterpretationCh 3,54 16-Feb 5 The Digital Image I Ch 4,10 18-Feb The Digital Image II5 23-Feb 6 Applications with areal and space photography 25-Feb Exam 1 26-Feb Lab 1 Introduction to ENVI – manipulation of digital imagery

  3. Our atmosphere

  4. Key components of VIS/RIR remote sensing 2. Energy emitted from sun based on Stephan/Boltzman Law, Planck’s formula, and Wein Displacement Law (Lecture 2) 1. Sun is EM Energy Source VIS/NIR Satellite EM energy EM energy 3. EM Energy interacts with the atmosphere 5. EM Energy interacts with the atmosphere Lecture 3 4.EM energy reflected from Earth’s Surface – Lectures 7/8

  5. Lecture 3 Topics/Key Points • Key Atmospheric Constituents • Gases, water, particulate matter • Effects of the atmosphere on EM energy • Reflection, Absorption, Scattering, Transmittance • Atmospheric extinction and the attenuation coefficient • Net effects of the atmosphere on VIS/IR energy reaching the earth’s surface - atmospheric windows

  6. What do gases and particles in the atmosphere do to EM radiation? • Refraction • Reflection • Absorption • Scattering • Transmittance

  7. 90 km

  8. Key components of VIS/NIR remote sensing VIS/NIR Satellite EM energy EM energy • Constituents of the atmosphere that will interact with EM radiation • Gases – CO2, N2Ox, CH4, O2, O3 • Water – • Water vapor • Water droplets • Ice particles • Particulate matter – smoke, dust, other particles

  9. Atmospheric Gases Nitrogen – N2 – 78% Oxygen – O2 – 21% Argon – Ar – 1% H20 – 0 to 7% • Major atmospheric trace gases (less than 0.1% each) Carbon dioxide – CO2 Ozone – O3 Methane – CH4 Carbon Monoxide – CO Nitrous Oxide – N2Ox Chlorofluorocarbons (CFCs)

  10. Water in the atmosphere • Water is present in a variety of forms in the atmosphere • Gas/vapor, droplets (liquid and frozen), ice crystals • The physical state (e.g., gas, liquid, solid) and density of water determines the manner in which it reacts with EM radiation • The amount of water in the atmosphere is highly variable, depending on climatic processes and earth/atmosphere interactions, particularly the hydrologic cycle

  11. Impacts of atmospheric water • When water is present in the form of clouds, it totally blocks radiation in the visible/RIR region of the EM spectrum • In other forms, atmospheric water affects the absorption, scattering, and transmission of visible/RIR radiation through the atmosphere

  12. Water is continuously being added to and removed from the atmosphere in a variety of forms through the global water cycle This water strongly influences EM radiation is passing through the atmosphere – it is a very transient characteristic, e.g., it is always changing

  13. Particulate Matter • Inorganic and organic particles that have been suspended in the atmosphere from a variety of sources

  14. Sources of particulate matter Natural processes • Volcanic eruptions – ash and inorganic compounds (example - sulfur dioxide) • Dust storms – small soil particles (sand, silt, and clay) • Wildland fires – soot and ash • Biological processes – emissions of complex hydrocarbons • Sea mist – water in droplets blowing of the sea surface evaporates, leaving sea salts Human activities • Burning of fossil fuels – soot and inorganic compounds • Biomass burning – soot, ash

  15. Dust cloud south of Iceland Observed by MODIS

  16. Smoke plume over Eastern US observed by MODIS in July 2002 from Forest Fires (red dots) in Quebec

  17. Landsat Image of Mt. Pinatubo Eruption

  18. Temporal/spatial variability of atmospheric constituents • Particulate matter • Highly variable both spatially and temporally, driven by the hydrologic cycle • A regional phenomenon, dependent on sources • Corrections must be made to account for the impacts of particulate matter • Need to understand possible sources for particulate matter in the regions of interest

  19. Temporal/spatial variability of atmospheric constituents • Atmospheric water • Highly variable both spatially and temporally, driven by the hydrologic cycle • A global phenomenon • Corrections must be made to account for the impacts of atmospheric water • Need to understand how hydrologic cycle is influencing atmospheric water in the regions of study

  20. Temporal/spatial variability of atmospheric constituents Trace gases CO2 CO N2Ox CH4CFC’s • Generally well mixed throughout the atmosphere • Change in response to physical, biological and chemical processes • Except for CO2, Spatial/temporal variations do not influence radiation in the VIS/RIR region of the EM spectrum

  21. The bottom line!!! • The constituents of the atmosphere are highly variable both spatially and temporally • These constituents interact with EM energy • To perform quantitative analyses of satellite remote sensing imagery requires an understanding of and accounting for atmospheric effects • Sophisticated computer models have been developed to quantify the effects of the atmosphere and to normalize remote sensing data for its effects

  22. Lecture 3 Topics/Key Points • Key Atmospheric Constituents • Gases, water, particulate matter • Effects of the atmosphere on EM energy • Reflection, Absorption, Scattering, Transmittance • Atmospheric extinction and the attenuation coefficient • Net effects of the atmosphere on VIS/IR energy reaching the earth’s surface - atmospheric windows

  23. Basic EM energy/matter interactions Incident EM Radiation Reflection Scattering Refraction Absorption Transmittance

  24. What do gases and particles in the atmosphere do to EM radiation? • Reflection • Absorption • Scattering • Transmittance

  25. Reflectance – the process whereby incoming EM radiation is reflected off the surface of an object Incoming Radiation Outgoing Radiation

  26. Atmospheric Reflection • Reflection of EM energy in the Visible/RIR region of the EM spectrum occurs primarily from the tops of dense clouds • ~25% of incoming solar EM energy in this wavelength region is reflected by clouds • When clouds of particulate matter (e.g., smoke, dust, etc.) are particularly thick or dense, the reflection from the tops of these can also occur

  27. Absorption • The process by which EM radiant energy is absorbed by a molecule or particle and converted to another form of energy

  28. UV radiation

  29. Summary of atmospheric absorption • Some trace atmospheric gases are strong absorbers of EM energy, but this absorption is confined to specific wavelength regions • Water is a very strong absorber of EM energy in specific wavelength regions > 0.7 m • Atmospheric particles will absorb some EM energy – because they are large, they tend to absorb all wavelengths equally

  30. Scattering • The process whereby EM radiation is absorbed and immediately re-emitted by a particleor molecule – energy can be emitted in multiple-directions Incoming EM energy Scattered energy Note: No EM energy is lost during scattering

  31. Types of Scattering • Rayleigh scattering • Mie scattering • Non-selective scattering The type of scattering is controlled by the size of the wavelength relative to the size of the particle

  32. Rayleigh Scattering(also called molecular scattering) Occurs when the wavelength λ>> the particle size

  33. Rayleigh scattering ~ 1 / 4 Rayleigh scattering occurs at a molecular level Through Rayleigh scattering, blue light (0.4 um) is scattered 5 times as much as red light (0.6 um)

  34. 90 km Most Rayleigh scattering occurs in the top 10 km of the stratosphere, e.g., at the ozone layer

  35. The clear sky appears blue because Rayleigh scattering high in the atmosphere influence short wavelength (blue) radiation the most Note UV radiation is not scattered by the upper atmosphere because it is absorbed by the OZONE Layer For further discussion of this slide, see http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html#c5

  36. Summary of Rayleigh Scattering • Occurs at the molecular level • The degree of Rayleigh scattering is inversely proportional to the fourth power of the EM wavelength • Most Rayleigh scattering occurs in the upper 10 km of the stratosphere

  37. Mie Scattering Occurs when the wavelength  particle size

  38. Mie Scattering • Occurs with particles that are actually 0.1 to 10 times the size of the wavelength • Primary Mie scatterers are dust particles, soot from smoke • Mie scatterers are found lower in the Troposphere

  39. Where does Mie Scattering Occur? The sources of Mie scatterers are at the earth’s surface, therefore, Mie scatterers are largely confined to the lower troposphere The exception are volcanoes, whose plumes of particulate matter are lifted well above the tropopause into the lower stratosphere

  40. Non-Selective Scattering Occurs when the wavelength << particle size

  41. Non-Selective Scattering • Its name derives from the fact that all wavelengths (visible/near IR) are equally affected • Particles are very large, typically water droplets and ice crystals of fog banks and clouds • Particles are 10 times the size of the wavelength, e.g., > 20 um in size

  42. For further discussion of this slide, see http://hyperphysics.phy-astr.gsu.edu/hbase/atmos/blusky.html#c5

  43. What do gases and particles in the atmosphere do to EM radiation? • Refraction • Reflection • Absorption • Scattering • Transmittance

  44. sun Reflected Refracted Scattered Absorbed Transmitted

  45. Atmospheric Transmittance • The fraction or percent of a particular frequency or wavelength of electromagnetic radiation that passes through the atmosphere without being reflected, absorbed or scattered.

  46. Lecture 3 Topics/Key Points • Key Atmospheric Constituents • Gases, water, particulate matter • Effects of the atmosphere on EM energy • Reflection, Absorption, Scattering, Transmittance • Atmospheric extinction and the attenuation coefficient • Net effects of the atmosphere on VIS/IR energy reaching the earth’s surface - atmospheric windows

  47. Atmospheric Extinction • Extinction is a term used to account for the loss or attenuation of radiant energy as light passes through the atmosphere, and includes both scattering and absorption • Extinction quantifies the amount of atmospheric transmittance

  48. Atmospheric Extinction Io - the unattenuated light intensity passing into the atmosphere L - the path length through the atmosphere I - attenuated light intensity

  49. Extinction Coefficient -  I / Io= e- L where I is the attenuated light intensity Io is the unattenuated light intensity L is the path length through the a uniform medium such as the atmosphere  is the extinction coefficient in the units of inverse distance

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