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Radiative Heat Transfer
Michael F. Modest
Manufacturer: Academic Press
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Similar Items:
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Thermal Radiation Heat Transfer
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Incompressible Flow
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Hypersonic and High Temperature Gas Dynamics (AIAA Education) (Aiaa Education Series)
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Fluid Mechanics, Third Edition
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ASIN: 0125031637 |
Book Description
Every chapter of Radiative Heat Transfer offers uncluttered nomenclature, numerous worked examples, and a large number of problems - many based on "real world" situations, making it ideal for classroom use as well as for self-study. The book's 22 chapters cover the four major areas in the field: surface properties; surface transport; properties of participating media; and transfer through participating media. Within each chapter, all analytical methods are developed in substantial detail, and a number of examples show how the developed relations may be applied to practical problems.
· Extensive solution manual for adopting instructors
· Most complete text in the field of radiative heat transfer
· Many worked examples and end-of-chapter problems
· Large number of computer codes (in Fortran and C++), ranging from basic problem solving aids to sophisticated research tools
· Covers experimental methods
Customer Reviews:
Especially commended to students of engineering.......2003-05-22
Now in an updated and expanded second edition, Radiative Heat Transfer by Michael F. Modest is a college-level mechanical and chemical engineering textbook, specifically written and intended for advanced students already familiar with basic calculus. Individual chapters address radiative exchange between a variety of surfaces; equations, functions, and methodologies; the influence of conduction and convention, and much, much more. An advanced resource and an excellent text or supplement to engineering education, Radiative Heat Transfer is especially commended to students of Mechanical Engineering and Chemical Engineering.
Book Description
Numerical Methods in Astrophysics: An Introduction outlines various fundamental numerical methods that can solve gravitational dynamics, hydrodynamics, and radiation transport equations. This resource indicates which methods are most suitable for particular problems, demonstrates what the accuracy requirements are in numerical simulations, and suggests ways to test for and reduce the inevitable negative effects. After an introduction to the basic equations and derivations, the book focuses on practical applications of the numerical methods. It explores hydrodynamic problems in one dimension, N-body particle dynamics, smoothed particle hydrodynamics, and stellar structure and evolution. The authors also examine advanced techniques in grid-based hydrodynamics, evaluate the methods for calculating the gravitational forces in an astrophysical system, and discuss specific problems in grid-based methods for radiation transfer. The book incorporates brief user instructions and a CD-ROM of the numerical codes, allowing readers to experiment with the codes to suit their own needs. With numerous examples and sample problems that cover a wide range of current research topics, this highly practical guide illustrates how to solve key astrophysics problems, providing a clear introduction for graduate and undergraduate students as well as researchers and professionals.
Customer Reviews:
Extremely good introduction!.......2007-09-22
This is an extremely well written introduction to a rapidly developing field. The authors cover a broad swath of topics, providing a clear understanding of the physical principles underlying numerical astrophysics. Such a focus on basic principles and physical understanding ensures that one does not lose sight of the forest for the trees. I recommend this book highly for graduate students in astrophysics, as well as active researchers in the field who want a quick overview before going into the details.
HUGE disappointment.......2007-04-08
I was really looking forward to this title, hoping in a book that would go beyond the usual toy problems of typical standard numerical simulations books. Also knowing that this book included real working code I was also hoping it would bridge the huge gap between theory and practice with a practical approach. Boy, was I mistaken. hard to believe, but there is not a single line of code in this book! The numerical codes in Fortran (yuk) are just dumped in the CD and superficially described (just barely saying what it does and what the input and output are) in a final 10 pages ( yes, you read that well, 10 pages) "chapter" that looks more like an appendix to anyone with a little common sense. I know college professors can be a bit disoriented about what is important and what not in their field of research (I still my quantum mechanics prof. employed approximately the same time to try to explain us while there are 2n+1 numbers between n and -n and to introduce us to Fourier Transforms) but this is really too much! The bunch of theory and equations that this book is littered is totally useless unless you show me how these equations get implemented in code.
And if I have to wade through the code in a CD trying to figure it out by myself, what is the value of buying this book? Given this approach , I really pity the grad students of these guys...
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A Monte Carlo Primer: A Practical Approach to Radiation Transport
Stephen A. Dupree , and
Stanley K. Fraley
Manufacturer: Springer
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Monte Carlo Primer: Volume 2
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Monte Carlo
ASIN: 0306467488 |
Book Description
This book introduces the reader to the use of Monte Carlo methods for solving practical problems in radiation transport, and will also serve as a reference work for practitioners in the field. It assumes the reader has a general knowledge of calculus and radiation physics, and a knowledge of Fortran programming, but assumes no prior knowledge of stochastic methods or statistical physics. The subject is presented by a combination of theoretical development and practical calculations. Because Monte Carlo methods are closely linked to the use of computers, from the beginning the reader is taught to convert the theoretical constructs developed in the text into functional software for use on a personal computer. Example problems provide the reader with an in-depth understanding of the concepts presented and lead to the production of a unique learning tool, a probabilistic framework code that models in a simple manner the features of production of Monte Carlo transport codes. This framework code is developed in stages such that every function is understood, tested, and demonstrated - random sampling, generating random numbers, implementing geometric models, using variance reduction, tracking particles in a random walk, testing the thoroughness with which the problem phase space is sampled, scoring detectors, and obtaining estimates of uncertainty in results. Advanced topics covered include criticality, correlated sampling, adjoint transport, and neutron thermalization.
Monte Carlo codes can produce highly precise wrong answers. The probability of this occurring is increased if production codes are run as opaque, `black boxes' of software. This text attempts to make Monte Carlo into a comprehensible, usable tool for solving practical transport problems. It is suitable for advanced undergraduate and graduate students and researchers who wish to expand their knowledge of the Monte Carlo technique.
Book Description
This volume provides a thorough and up-to-date treatment of multiple scattering of light and other electromagnetic radiation in media composed of randomly and sparsely positioned particles. It systematically and consistently presents radiative transfer theory as a branch of classical macroscopic electromagnetics. After tracing the fundamental link between radiative transfer theory and the effect of coherent backscattering, the authors explain them in the context of a comprehensive hierarchy of electromagnetic scattering problems. Dedicated sections present a thorough discussion of the physical meaning and range of applicability of the radiative transfer equation and compare the self-consistent microphysical and the traditional phenomenological approaches to radiative transfer. This self-contained book will be valuable for science professionals, engineers, and graduate students working across a wide range of disciplines including optics, electromagnetics, remote sensing, atmospheric radiation, astrophysics, and biomedicine.
Book Description
Foundation for analysis of stellar atmospheres, planetary illumination, sky radiation; physical interest for problems analogous to diffusion of neutrons.
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Non-LTE Radiative Transfer in the Atmosphere, (Series on Atmospheric, Ocean and Planetary Physics, Vol. 3) (Series on Atmospheric, Oceanic and Planetary Physics)
M. Lopez-Puertas ,
F. W. Taylor , and
M. Lopez Puertas
Manufacturer: World Scientific Publishing Company
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Binding: Hardcover
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ASIN: 9810245661 |
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3D Radiative Transfer in Cloudy Atmospheres (Physics of Earth and Space Environments)
Manufacturer: Springer
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ASIN: 3540239588 |
Book Description
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.
Book Description
This text provides a foundation in both the theoretical and practical aspects of radiative transfer, for advanced students of atmospheric, oceanic and environmental sciences. The transfer of solar and infrared radiation through optically-thick clouds, aerosol layer, and the oceanic mixed layer is presented through the use of heuristic models of scattering and absorption, and a systematic approach to formulation and solution of the radiative transfer equation. Problems such as the the transmission of ultraviolet radiation through the atmosphere and ocean, remote sensing, solar heating and infrared cooling processes, UV biological dose rates, and Greenhouse warming are solved using a variety of methods. This self-contained, systematic treatment will prepare students from a range of disciplines in problems concerning the effects of solar and infrared radiation on natural systems. The hardback edition received excellent reviews.
Customer Reviews:
Solid science.......2007-09-30
Excellent, clear textbook! Very valuable for those who wish to discuss climate change intelligently. Extremely valuable for those who are attarcted to the improbable hypotheses of Svensmark.
one of the best textbooks that I ever read.......2006-03-24
This is really a talk-to-student text book, especially among the ones of radiative transfer topic. It reads much easier than Goody's. Also more updated and providing more pracitical guidance for those who want to write up a small program to test out some theories and those serious ones, like atmospheric radiative transfer majors.
I do find quite a few typos and mistakes in equations that are still not corrected in their online errata. The denotation letters are a bit confusing, but no worse than the other ones.
I would recommend it to beginners definitely!
Great physical insight solving radiative transfer problems.......2002-12-19
This text covers a broad range of topics in radiative transfer with clarity and style. What is particularly appreciated is that the text not only provides detailed solutions to radiative transfer problems, but discusses their weaknesses and strengths in practical applications, and also provides unusual insight into their physical meaning. My only complaint is that the notation is somewhat unconventional (for example the single-scattering albedo is represented by 'a'), and this takes some getting used to.
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High Temperature Gas Dynamics
Tarit K. Bose
Manufacturer: Springer
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ASIN: 3540408851 |
Book Description
High Temperature Gas Dynamics is a class-tested primer for students, scientists and engineers who would like to have a basic understanding of the physics and the behaviour of high-temperature gases. It is a valuable tool for astrophysicists as well. The first chapters treat the basic principles of quantum and statistical mechanics and how to derive thermophysical properties from them. Special topics are included that are rarely found in other textbooks, such as the thermophysical and transport properties of multi-temperature gases and a novel method to compute radiative transfer. Furthermore, collision processes between different particles are discussed. Separate chapters deal with the production of high-temperature gases and with electrical emission in plasmas, as well as related diagnostic techniques.
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