Numerical Modeling In Applied Physics And Astrophysics

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Numerical Modeling in Applied Physics and Astrophysics

Author : Richard L. Bowers,James Ricker Wilson
Publisher : Jones & Bartlett Publishers
Page : 730 pages
File Size : 50,8 Mb
Release : 1991
Category : Science
ISBN : UCAL:B4359620

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Numerical Modeling in Applied Physics and Astrophysics by Richard L. Bowers,James Ricker Wilson Pdf

Introduction to Numerical Modeling in Engineering and Applied Physics

Author : Peter L. Hagelstein
Publisher : Wiley
Page : 900 pages
File Size : 46,6 Mb
Release : 2019-03-25
Category : Technology & Engineering
ISBN : 0471715743

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Introduction to Numerical Modeling in Engineering and Applied Physics by Peter L. Hagelstein Pdf

Presenting material used extensively by students at MIT where the author teaches, Introduction to Numerical Modeling in Engineering and Applied Physics which allows students and professionals access to basic methods and approaches in numerical simulations, so that they will be able to develop their own numerical models and better understand numerical models developed by others. It assumes no previous experience with numerical modeling, and is addressed to scientists and engineers in engineering and applied physics who are involved in modeling, covering a broad range of generally useful numerical methods and algorithms from a user-oriented perspective.

Numerical Modelling of Astrophysical Turbulence

Author : Wolfram Schmidt
Publisher : Springer Science & Business Media
Page : 98 pages
File Size : 50,8 Mb
Release : 2013-09-20
Category : Science
ISBN : 9783319014753

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Numerical Modelling of Astrophysical Turbulence by Wolfram Schmidt Pdf

In this "SpringerBrief" the author considers the underlying problems and questions that are common to numerical models of turbulence in different astrophysical systems. Turbulence has emerged as an important research topic in several areas of astrophysics. Understanding and modeling turbulence is particularly important for the dynamics of the interstellar medium, but also for the intergalactic medium, as well as in stars. The advancement of methods for numerical simulations of astrophysical turbulence, however, is still challenging because of gravity, strong compressibility, magnetic fields, and other effects. The book begins with a review of general aspects of numerical simulations of turbulence. In the main part the author presents findings from his numerical studies on astrophysical turbulence and discusses the astrophysical implications. He also explains in detail the numerical schemes utilized. Readers will find that this book offers a compact yet comprehensive introduction.

Numerical Methods in Astrophysics

Author : Peter Bodenheimer,Gregory P. Laughlin,Michal Rozyczka,Tomasz Plewa,Harold. W Yorke,Harold W. Yorke
Publisher : Taylor & Francis
Page : 344 pages
File Size : 52,8 Mb
Release : 2006-12-13
Category : Science
ISBN : 9781420011869

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Numerical Methods in Astrophysics by Peter Bodenheimer,Gregory P. Laughlin,Michal Rozyczka,Tomasz Plewa,Harold. W Yorke,Harold W. Yorke Pdf

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, a

Numerical Methods in Astrophysics

Author : Peter Bodenheimer,Gregory P. Laughlin,Michal Rozyczka,Tomasz Plewa,Harold. W Yorke,Harold W. Yorke
Publisher : CRC Press
Page : 360 pages
File Size : 54,7 Mb
Release : 2006-12-13
Category : Science
ISBN : 0750308834

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Numerical Methods in Astrophysics by Peter Bodenheimer,Gregory P. Laughlin,Michal Rozyczka,Tomasz Plewa,Harold. W Yorke,Harold W. Yorke Pdf

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.

The Numerical Modelling of Nonlinear Stellar Pulsations

Author : J. Robert Buchler
Publisher : Springer Science & Business Media
Page : 372 pages
File Size : 49,5 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400905191

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The Numerical Modelling of Nonlinear Stellar Pulsations by J. Robert Buchler Pdf

This interdisciplinary meeting has brought together a group of astrophysicists with hands-on experience in the numerical computation of astrophysical fluid dynamics, in particular nonlinear stellar pulsations, and a group of applied mathematicians who are actively engaged with the development of novel and improved numerical methods. The goal of the workshop has been for the astrophysicists to discuss in detail the numerical problems encountered in the modelling of stellar pulsations and for the mathematicians to present a survey of recent developments in numerical techniques. This astrophysical-mathematical intercourse will help the astrophysicists in the future development of more reliable and efficient codes, on the one hand, and it has introduced the mathematicians to an unfamiliar area which is a tough testing ground for their techniques. Since the difficulties encountered are common to other fluid dynamics problems, and are in fact perhaps more severe, fluid dynamicists in other research areas may fmd the results of this workshop of interest as well. Much of our theoretical understanding of the intricate and interesting behavior of variable stars rests on our ability to perform accurate numerical hydrodynamical computations of stellar models. Extensive calculations of nonlinear radial stellar pulsations with the use of increasingly powerful computers are showing more and more clearly that the numerical codes in current use have serious deficiencies.

Physics of the Sun

Author : Dermott J. Mullan
Publisher : CRC Press
Page : 384 pages
File Size : 49,9 Mb
Release : 2009-08-26
Category : Science
ISBN : 9781420083088

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Physics of the Sun by Dermott J. Mullan Pdf

With an emphasis on numerical modeling, Physics of the Sun: A First Course presents a quantitative examination of the physical structure of the Sun and the conditions of its extended atmosphere. It gives step-by-step instructions for calculating the numerical values of various physical quantities.The text covers a wide range of topics on the Sun an

Astrophysics through Computation

Author : Brian Koberlein,David Meisel
Publisher : Cambridge University Press
Page : 385 pages
File Size : 43,6 Mb
Release : 2013-06-28
Category : Science
ISBN : 9781107276451

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Astrophysics through Computation by Brian Koberlein,David Meisel Pdf

This new text surveys a series of fundamental problems in astrophysics, both analytically and computationally, for advanced students in physics and astrophysics. The contents are supported by more than 110 class-tested Mathematica® notebooks, allowing rigorous solutions to be explored in a visually engaging way. Topics covered include many classical and historically interesting problems, enabling students to appreciate the mathematical and scientific challenges that have been overcome in the subject's development. The text also shows the advantages and disadvantages of using analytical and computational methods. It will serve students, professionals and capable amateurs to master the quantitative details of modern astrophysics and the computational aspects of their research projects. Downloadable Mathematica® resources available at www.cambridge.org/koberlein.

Frontiers And Prospects Of Contemporary Applied Mathematics

Author : Pingwen Zhang,Tatsien Li
Publisher : World Scientific
Page : 276 pages
File Size : 48,8 Mb
Release : 2006-04-17
Category : Mathematics
ISBN : 9789814478519

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Frontiers And Prospects Of Contemporary Applied Mathematics by Pingwen Zhang,Tatsien Li Pdf

This collection of articles covers the hottest topics in contemporary applied mathematics. Multiscale modeling, material computing, symplectic methods, parallel computing, mathematical biology, applied differential equations and engineering computing problems are all included. The book contains the latest results of many leading scientists and provides a window on new trends in research in the field.

Numerical Recipes in FORTRAN 77: Volume 1, Volume 1 of Fortran Numerical Recipes

Author : William H. Press,Saul A. Teukolsky,Brian P. Flannery,William T. Vetterling
Publisher : Cambridge University Press
Page : 1016 pages
File Size : 42,5 Mb
Release : 1992-09-25
Category : Computers
ISBN : 052143064X

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Numerical Recipes in FORTRAN 77: Volume 1, Volume 1 of Fortran Numerical Recipes by William H. Press,Saul A. Teukolsky,Brian P. Flannery,William T. Vetterling Pdf

As with Numerical Recipes in C, the FORTRAN edition has been greatly revised to make this edition the most up to date handbook for those working with FORTRAN. Between both editions of Numerical Recipes, over 300,000 copies have been sold.

Computational Methods for Astrophysical Fluid Flow

Author : Randall J. LeVeque,Dimitri Mihalas,E.A. Dorfi,Ewald Müller
Publisher : Springer Science & Business Media
Page : 523 pages
File Size : 52,5 Mb
Release : 2006-04-18
Category : Science
ISBN : 9783540316329

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Computational Methods for Astrophysical Fluid Flow by Randall J. LeVeque,Dimitri Mihalas,E.A. Dorfi,Ewald Müller Pdf

This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures.

High-Resolution Methods for Incompressible and Low-Speed Flows

Author : D. Drikakis,W. Rider
Publisher : Springer Science & Business Media
Page : 622 pages
File Size : 49,8 Mb
Release : 2006-03-30
Category : Science
ISBN : 9783540264545

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High-Resolution Methods for Incompressible and Low-Speed Flows by D. Drikakis,W. Rider Pdf

The study of incompressible ?ows is vital to many areas of science and te- nology. This includes most of the ?uid dynamics that one ?nds in everyday life from the ?ow of air in a room to most weather phenomena. Inundertakingthesimulationofincompressible?uid?ows,oneoftentakes many issues for granted. As these ?ows become more realistic, the problems encountered become more vexing from a computational point-of-view. These range from the benign to the profound. At once, one must contend with the basic character of incompressible ?ows where sound waves have been analytically removed from the ?ow. As a consequence vortical ?ows have been analytically “preconditioned,” but the ?ow has a certain non-physical character (sound waves of in?nite velocity). At low speeds the ?ow will be deterministic and ordered, i.e., laminar. Laminar ?ows are governed by a balance between the inertial and viscous forces in the ?ow that provides the stability. Flows are often characterized by a dimensionless number known as the Reynolds number, which is the ratio of inertial to viscous forces in a ?ow. Laminar ?ows correspond to smaller Reynolds numbers. Even though laminar ?ows are organized in an orderly manner, the ?ows may exhibit instabilities and bifurcation phenomena which may eventually lead to transition and turbulence. Numerical modelling of suchphenomenarequireshighaccuracyandmostimportantlytogaingreater insight into the relationship of the numerical methods with the ?ow physics.

Literature 1991, Part 2

Author : Astronomisches Rechen-Institut
Publisher : Springer Science & Business Media
Page : 1592 pages
File Size : 51,7 Mb
Release : 2013-06-29
Category : Science
ISBN : 9783662123768

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Literature 1991, Part 2 by Astronomisches Rechen-Institut Pdf

"Astronomy and Astrophysics Abstracts" appearing twice a year has become oneof the fundamental publications in the fields of astronomy, astrophysics andneighbouring sciences. It is the most important English-language abstracting journal in the mentioned branches. The abstrats are classified under more than a hundred subject categories, thus permitting a quick survey of the whole extended material. The AAA is a valuable and important publication for all students and scientists working in the fields of astronomy and related sciences. As such it represents a necessary ingredient of any astronomical library all over the world.

Analog Circuit Simulators for Integrated Circuit Designers

Author : Mikael Sahrling
Publisher : Springer Nature
Page : 414 pages
File Size : 42,7 Mb
Release : 2021-03-26
Category : Technology & Engineering
ISBN : 9783030642068

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Analog Circuit Simulators for Integrated Circuit Designers by Mikael Sahrling Pdf

Learn how analog circuit simulators work with these easy to use numerical recipes implemented in the popular Python programming environment. This book covers the fundamental aspects of common simulation analysis techniques and algorithms used in professional simulators today in a pedagogical way through simple examples. The book covers not just linear analyses but also nonlinear ones like steady state simulations. It is rich with examples and exercises and many figures to help illustrate the points. For the interested reader, the fundamental mathematical theorems governing the simulation implementations are covered in the appendices. Demonstrates circuit simulation algorithms through actual working code, enabling readers to build an intuitive understanding of what are the strengths and weaknesses with various methods Provides details of all common, modern circuit simulation methods in one source Provides Python code for simulations via download Includes transistor numerical modeling techniques, based on simplified transistor physics Provides detailed mathematics and ample references in appendices

Theoretical and Observational Problems Related to Solar Eclipses

Author : Z. Mouradian,Magda Stavinschi
Publisher : Springer Science & Business Media
Page : 264 pages
File Size : 52,6 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789401154925

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Theoretical and Observational Problems Related to Solar Eclipses by Z. Mouradian,Magda Stavinschi Pdf

The NATO ARW on the problems of ground-based observations of Solar Eclipses was held in Sinaia (Romania) between 1 and 5 June 1996. The Workshop was divided into seven sessions, in which 17 papers were given, by key speakers, along with 30 oral presentations. Additionally, 30 posters were presented. This issue contains only the invited and oral papers. The posters are to be published in a special issue of the Romanian Astronomical Journal. The contributions were based on our present knowledge of solar corona physics and on the perspectives for future total eclipse observations, focussing especially on that of August 11, 1999, which will be the last eclipse of the century. The workshop sessions reviewed the results of past eclipse observations, coronal hot and cold structures, coronal heating, public education, and instrumental problems. At the end of the meeting a fruitful general discussion drew out problems to be studied and techniques to be used for forthcoming observations. Posters completed the workshop contributions.