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

Product form

£54.86

Includes FREE delivery

RRP £60.95 – you save £6.09 (9%)

Order before 4pm tomorrow for delivery by Sat 20 Dec 2025.

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

Out of stock


    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

    Recently viewed products

    © 2025 Book Curl

      • American Express
      • Apple Pay
      • Diners Club
      • Discover
      • Google Pay
      • Maestro
      • Mastercard
      • PayPal
      • Shop Pay
      • Union Pay
      • Visa

      Login

      Forgot your password?

      Don't have an account yet?
      Create account