Numerical Modelling of Astrophysical Turbulence: SpringerBriefs in Astronomy
Autor Wolfram Schmidten Limba Engleză Paperback – 7 oct 2013
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.
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Specificații
ISBN-13: 9783319014746
ISBN-10: 3319014749
Pagini: 100
Ilustrații: VIII, 90 p. 50 illus., 22 illus. in color.
Dimensiuni: 155 x 235 x 5 mm
Greutate: 0.16 kg
Ediția:2014
Editura: Springer International Publishing
Colecția Springer
Seria SpringerBriefs in Astronomy
Locul publicării:Cham, Switzerland
ISBN-10: 3319014749
Pagini: 100
Ilustrații: VIII, 90 p. 50 illus., 22 illus. in color.
Dimensiuni: 155 x 235 x 5 mm
Greutate: 0.16 kg
Ediția:2014
Editura: Springer International Publishing
Colecția Springer
Seria SpringerBriefs in Astronomy
Locul publicării:Cham, Switzerland
Public țintă
ResearchCuprins
Turbulence theory.- Simulation techniques.- Phenomenology and statistics.- Complex processes.
Recenzii
“This book provides an interesting and well-written account on an area witnessing encouraging progress.” (H. Muthsam, Monatshefte für Mathematik, 2016)
“The primary focus of this book is on the numerical methods and their application in studying the fundamental statistical properties of compressible hydrodynamic turbulence. … The book can be a useful survey and reference source for researchers in the field. Also, it can be a good point of introduction for someone wanting to develop a research capability in this area.” (Stephen Wollman, zbMATH 1317.85004, 2015)
“The primary focus of this book is on the numerical methods and their application in studying the fundamental statistical properties of compressible hydrodynamic turbulence. … The book can be a useful survey and reference source for researchers in the field. Also, it can be a good point of introduction for someone wanting to develop a research capability in this area.” (Stephen Wollman, zbMATH 1317.85004, 2015)
Textul de pe ultima copertă
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.
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.
Caracteristici
Provides a compact and comprehensive introduction into a subject which is usually covered only in research papers or advanced and lengthy textbooks Disparate areas of astrophysics with traditionally separate communities are linked by the same underlying physics Informs about frontiers of supercomputing in astrophysics Includes supplementary material: sn.pub/extras