3D Radiative Transfer in Cloudy Atmospheres

3D Radiative Transfer in Cloudy Atmospheres
Author: Alexander Marshak
Publisher: Springer Science & Business Media
Total Pages: 688
Release: 2006-05-27
Genre: Science
ISBN: 3540285199

Developments in three-dimensional cloud radiation over the past few decades are assessed and distilled into this contributed volume. Chapters are authored by subject-matter experts who address a broad audience of graduate students, researchers, and anyone interested in cloud-radiation processes in the solar and infrared spectral regions. After two introductory chapters and a section on the fundamental physics and computational techniques, the volume extensively treats two main application areas: the impact of clouds on the Earth's radiation budget, which is an essential aspect of climate modeling; and remote observation of clouds, especially with the advanced sensors on current and future satellite missions.

Three-Dimensional Radiative Transfer Modeling of Tropospheric Atmospheres

Three-Dimensional Radiative Transfer Modeling of Tropospheric Atmospheres
Author: United States. Army Research Laboratory
Publisher:
Total Pages: 126
Release: 1998-03-01
Genre:
ISBN: 9781423563075

Physically accurate visualizations of tropospheric atmospheres require three-dimensional (3D) radiative transfer (RT) codes capable of simulating scattering and absorption effects in and around natural clouds. This report describes an adaptation of the discrete ordinates technique for handling both thin (haze) and thick (natural cloud) optical media in a consistent manner. Media are modeled via uniform density cubical scattering cells (assuming that incident diffuse streams have uniform radiance over each input face). These assumptions allow the analytic evaluation of transmission factors and volume- averaged unscat- tered illumination across a cell in evaluating scattered streaming energies at each cell exit face. This initial analysis leads to an energy accounting technique which replaces energy not accounted for via transmission and diffuse single scattering with a surface scattering effect. Solar/lunar direct irradiance and graybody radiation are also considered. Monte Carlo analyses were used to determine the accuracy of the proposed methods. Path point-to-point calculations are described that adapt the outputs of the RT code to provide limiting path radiance information for visualization of could fields. An analysis of the scattering properties of aerosols as scale transformed Legendre polynomial expansions is also provided.

Radiation Heat Transfer Modelling with Computational Fluid Dynamics

Radiation Heat Transfer Modelling with Computational Fluid Dynamics
Author: Yehuda Sinai
Publisher: CRC Press
Total Pages: 214
Release: 2022-06-20
Genre: Science
ISBN: 1000567044

This book serves as a preliminary reference for the principles of thermal radiation and its modelling in computational fluid dynamics (CFD) simulations. Radiation Heat Transfer Modelling with Computational Fluid Dynamics covers strategies and processes for synthesizing radiation with CFD setups, computational techniques for solving the radiative transfer equation, the strengths and weaknesses thereof, boundary and initial conditions and relevant guidelines. Describing the strategic planning of a typical project, the book includes the spectroscopic properties of gases, some particulates and porous media. FEATURES Fills a gap between existing CFD and thermal radiation textbooks and elaborates on some aspects of user manuals. Aims at (1) CFD practitioners who are newcomers to thermal radiation and are looking for a preliminary introduction thereon and (2) modellers familiar with thermal radiation looking for a precursory introduction to CFD. The book is tilted somewhat towards the first group. Provides guidelines for choosing the right model, the strategic planning of the modelling and its implementation. Outlines the pitfalls of some solution techniques. Describes how radiation is included in the variety of boundary condition types offered by CFD codes. Helps to develop the practical skills required to plan, implement and interpret thermal radiation within the typical CFD code. Addresses a wide variety of physical circumstances in which thermal radiation plays a role. Offers ample references for readers searching for additional details. Includes several examples of practical applications, including fire, a utility boiler and car headlights in cold environments. This book is intended for researchers and professionals who wish to simulate problems that involve fluid flow and heat transfer with thermal radiation.

The Monte Carlo Methods in Atmospheric Optics

The Monte Carlo Methods in Atmospheric Optics
Author: G.I. Marchuk
Publisher: Springer
Total Pages: 210
Release: 2014-10-05
Genre: Technology & Engineering
ISBN: 9783662135020

This monograph is devoted to urgent questions of the theory and applications of the Monte Carlo method for solving problems of atmospheric optics and hydrooptics. The importance of these problems has grown because of the increas ing need to interpret optical observations, and to estimate radiative balance precisely for weather forecasting. Inhomogeneity and sphericity of the atmos phere, absorption in atmospheric layers, multiple scattering and polarization of light, all create difficulties in solving these problems by traditional methods of computational mathematics. Particular difficulty arises when one must solve nonstationary problems of the theory of transfer of narrow beams that are connected with the estimation of spatial location and time characteristics of the radiation field. The most universal method for solving those problems is the Monte Carlo method, which is a numerical simulation of the radiative-transfer process. This process can be regarded as a Markov chain of photon collisions in a medium, which result in scattering or absorption. The Monte Carlo tech nique consists in computational simulation of that chain and in constructing statistical estimates of the desired functionals. The authors of this book have contributed to the development of mathemati cal methods of simulation and to the interpretation of optical observations. A series of general method using Monte Carlo techniques has been developed. The present book includes theories and algorithms of simulation. Numerical results corroborate the possibilities and give an impressive prospect of the applications of Monte Carlo methods.

The Atmosphere and Climate of Mars

The Atmosphere and Climate of Mars
Author: Robert M. Haberle
Publisher: Cambridge University Press
Total Pages: 613
Release: 2017-06-29
Genre: Science
ISBN: 110817938X

Humanity has long been fascinated by the planet Mars. Was its climate ever conducive to life? What is the atmosphere like today and why did it change so dramatically over time? Eleven spacecraft have successfully flown to Mars since the Viking mission of the 1970s and early 1980s. These orbiters, landers and rovers have generated vast amounts of data that now span a Martian decade (roughly eighteen years). This new volume brings together the many new ideas about the atmosphere and climate system that have emerged, including the complex interplay of the volatile and dust cycles, the atmosphere-surface interactions that connect them over time, and the diversity of the planet's environment and its complex history. Including tutorials and explanations of complicated ideas, students, researchers and non-specialists alike are able to use this resource to gain a thorough and up-to-date understanding of this most Earth-like of planetary neighbours.

Radiative Processes in Astrophysics

Radiative Processes in Astrophysics
Author: George B. Rybicki
Publisher: John Wiley & Sons
Total Pages: 400
Release: 2008-09-26
Genre: Science
ISBN: 352761818X

Radiative Processes in Astrophysics: This clear, straightforward, and fundamental introduction is designed to present-from a physicist's point of view-radiation processes and their applications to astrophysical phenomena and space science. It covers such topics as radiative transfer theory, relativistic covariance and kinematics, bremsstrahlung radiation, synchrotron radiation, Compton scattering, some plasma effects, and radiative transitions in atoms. Discussion begins with first principles, physically motivating and deriving all results rather than merely presenting finished formulae. However, a reasonably good physics background (introductory quantum mechanics, intermediate electromagnetic theory, special relativity, and some statistical mechanics) is required. Much of this prerequisite material is provided by brief reviews, making the book a self-contained reference for workers in the field as well as the ideal text for senior or first-year graduate students of astronomy, astrophysics, and related physics courses. Radiative Processes in Astrophysics also contains about 75 problems, with solutions, illustrating applications of the material and methods for calculating results. This important and integral section emphasizes physical intuition by presenting important results that are used throughout the main text; it is here that most of the practical astrophysical applications become apparent.

An Introduction to Atmospheric Radiation

An Introduction to Atmospheric Radiation
Author: K. N. Liou
Publisher: Academic Press
Total Pages: 599
Release: 2002-04-29
Genre: Nature
ISBN: 0124514510

Fundamentals of radiation for atmospheric applications -- Solar radiation at the top of the atmosphere -- Absorption and scattering of solar radiation in the atmosphere -- Thermal infrared radiation transfer in the atmosphere -- Light scattering by atmospheric particulates -- Principles of radiative transfer in planetary atmospheres -- Application of radiative transfer principles to remote sensing -- Radiation and climate.

The Monte Carlo Methods in Atmospheric Optics

The Monte Carlo Methods in Atmospheric Optics
Author: G.I. Marchuk
Publisher: Springer
Total Pages: 218
Release: 2013-04-17
Genre: Science
ISBN: 3540352376

This monograph is devoted to urgent questions of the theory and applications of the Monte Carlo method for solving problems of atmospheric optics and hydrooptics. The importance of these problems has grown because of the increas ing need to interpret optical observations, and to estimate radiative balance precisely for weather forecasting. Inhomogeneity and sphericity of the atmos phere, absorption in atmospheric layers, multiple scattering and polarization of light, all create difficulties in solving these problems by traditional methods of computational mathematics. Particular difficulty arises when one must solve nonstationary problems of the theory of transfer of narrow beams that are connected with the estimation of spatial location and time characteristics of the radiation field. The most universal method for solving those problems is the Monte Carlo method, which is a numerical simulation of the radiative-transfer process. This process can be regarded as a Markov chain of photon collisions in a medium, which result in scattering or absorption. The Monte Carlo tech nique consists in computational simulation of that chain and in constructing statistical estimates of the desired functionals. The authors of this book have contributed to the development of mathemati cal methods of simulation and to the interpretation of optical observations. A series of general method using Monte Carlo techniques has been developed. The present book includes theories and algorithms of simulation. Numerical results corroborate the possibilities and give an impressive prospect of the applications of Monte Carlo methods.