Description

Book Synopsis
This textbook is a first-look at radiative transfer in planetary atmospheres with a particular focus on the Earth's atmosphere and climate. It covers the basics of the radiative transfer of sunlight, treating absorption and scattering, and the transfer of the thermal infrared. The examples included show how the solutions of the radiative transfer equation are used to evaluate changes in the Earth?s energy budget due to changes in atmospheric composition, how these changes lead to climate change, and also how remote sensing can be used to probe the thermal structure and composition of planetary atmospheres. The examples motivate students by leading them to a better understanding of and appreciation for the computer-generated numerical results.
Aimed at upper-division undergraduates and beginning graduate students in physics and atmospheric sciences, the book is designed to cover the essence of the material in a 10-week course, while the material in the optional sections will facilitate its use at the more leisurely pace and in-depth focus of a semester course.


Table of Contents
SIMPLE MODELS FOR THE RADIATIVE HAETING OF THE EARTH AND ITS ATMOSPHERE
Introduction
Radiative Heating of the Atmosphere
Global Energy Budget
The Window-Gray Approximation and the Greenhouse Effect
Climate Sensitivity
Radiative Time Constant
Radiation and the Earth's Global Mean Vertical Temperature Profile
Radiative Forcding Leads to Circulation
RADIATION AND ITS SOURCES
Basic Properties of Electromagnetic Wave
Wave-Particle Duality of Light
Blackbody Radiation
Incident Sunlight
TRANSFER OF RADIATION IN THE EARTH'S ATMOSPHERE
Cross Sections
Extinction Cross Section and Scattering Phase Function
Atmospheric Optical Phenomena Related to Light Scattering
Equation of Radiative Transfer
Transfer Equation for Solar Radiation
Transfer Equation for Terrestrial Radiation
SOLUTIONS TO THE EQUATION OF TRANSFER
Formal Solution to the Equation of Transfer
Solution for Thermal Emission
Solution for Scattering and Absorption
Single-Scattering Approximation
Fourier Decomposition of the Transfer Equation
Eddington Approximation for Scattering and Absorbing Atmosphere
Adding Layers in the Eddington Approximation
Adding a Surface with a Nonzero Albedo in the Eddington Approximation
Clouds in the Thermal Infrared
Diffusivity Factor
TREATMENT OF MOLECULAR ABSORPTION IN THE ATMOSPHERE
Absorption by Molecules
Molecular Absorption Lines and Line Shapes
Molecular Absorption Spectra
Distribution of Line Strengths for a Vibration Rotation Band
Absorption by a Single, Weak Absorption Line
Absorption by a Single, Strong, Pressure-Broadened Line
Inhomogeneous Ppaths
Bands of Isolated Lines
Approximate Treatments for Overlapping Lines
Exponential Sum-Fit and Correlated-K Methods
ABSORBTION OF SOLRA RADIATION IN THE EARTH'S ATMOSPHERE
Absorption of UV and Visible Sunlight by Ozone
Absorption of Sunlight by Water Vapor
SIMPLIFIED ESTIMATES OF EMISSION
Emission in the 15-?m band of CO2
Change in Emitted Flux Due to a Doubling of CO2
Change in Stratospheric Temperature Due to a Doubling of CO2
APPENDICES
Solving Differential Equations
Integrals of the Planck Function
Compilation of Line Parameters for Random Band Models
Absorption Cross Sections for Ozone and Oxygen at Ultraviolet and Visible Wavelengths

Atmospheric Radiation: A Primer with Illustrative

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    A Paperback / softback by James A. Coakley Jr., Ping Yang

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      View other formats and editions of Atmospheric Radiation: A Primer with Illustrative by James A. Coakley Jr.

      Publisher: Wiley-VCH Verlag GmbH
      Publication Date: 16/07/2014
      ISBN13: 9783527410989, 978-3527410989
      ISBN10: 3527410988

      Description

      Book Synopsis
      This textbook is a first-look at radiative transfer in planetary atmospheres with a particular focus on the Earth's atmosphere and climate. It covers the basics of the radiative transfer of sunlight, treating absorption and scattering, and the transfer of the thermal infrared. The examples included show how the solutions of the radiative transfer equation are used to evaluate changes in the Earth?s energy budget due to changes in atmospheric composition, how these changes lead to climate change, and also how remote sensing can be used to probe the thermal structure and composition of planetary atmospheres. The examples motivate students by leading them to a better understanding of and appreciation for the computer-generated numerical results.
      Aimed at upper-division undergraduates and beginning graduate students in physics and atmospheric sciences, the book is designed to cover the essence of the material in a 10-week course, while the material in the optional sections will facilitate its use at the more leisurely pace and in-depth focus of a semester course.


      Table of Contents
      SIMPLE MODELS FOR THE RADIATIVE HAETING OF THE EARTH AND ITS ATMOSPHERE
      Introduction
      Radiative Heating of the Atmosphere
      Global Energy Budget
      The Window-Gray Approximation and the Greenhouse Effect
      Climate Sensitivity
      Radiative Time Constant
      Radiation and the Earth's Global Mean Vertical Temperature Profile
      Radiative Forcding Leads to Circulation
      RADIATION AND ITS SOURCES
      Basic Properties of Electromagnetic Wave
      Wave-Particle Duality of Light
      Blackbody Radiation
      Incident Sunlight
      TRANSFER OF RADIATION IN THE EARTH'S ATMOSPHERE
      Cross Sections
      Extinction Cross Section and Scattering Phase Function
      Atmospheric Optical Phenomena Related to Light Scattering
      Equation of Radiative Transfer
      Transfer Equation for Solar Radiation
      Transfer Equation for Terrestrial Radiation
      SOLUTIONS TO THE EQUATION OF TRANSFER
      Formal Solution to the Equation of Transfer
      Solution for Thermal Emission
      Solution for Scattering and Absorption
      Single-Scattering Approximation
      Fourier Decomposition of the Transfer Equation
      Eddington Approximation for Scattering and Absorbing Atmosphere
      Adding Layers in the Eddington Approximation
      Adding a Surface with a Nonzero Albedo in the Eddington Approximation
      Clouds in the Thermal Infrared
      Diffusivity Factor
      TREATMENT OF MOLECULAR ABSORPTION IN THE ATMOSPHERE
      Absorption by Molecules
      Molecular Absorption Lines and Line Shapes
      Molecular Absorption Spectra
      Distribution of Line Strengths for a Vibration Rotation Band
      Absorption by a Single, Weak Absorption Line
      Absorption by a Single, Strong, Pressure-Broadened Line
      Inhomogeneous Ppaths
      Bands of Isolated Lines
      Approximate Treatments for Overlapping Lines
      Exponential Sum-Fit and Correlated-K Methods
      ABSORBTION OF SOLRA RADIATION IN THE EARTH'S ATMOSPHERE
      Absorption of UV and Visible Sunlight by Ozone
      Absorption of Sunlight by Water Vapor
      SIMPLIFIED ESTIMATES OF EMISSION
      Emission in the 15-?m band of CO2
      Change in Emitted Flux Due to a Doubling of CO2
      Change in Stratospheric Temperature Due to a Doubling of CO2
      APPENDICES
      Solving Differential Equations
      Integrals of the Planck Function
      Compilation of Line Parameters for Random Band Models
      Absorption Cross Sections for Ozone and Oxygen at Ultraviolet and Visible Wavelengths

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