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Titlebook: Numerical Modelling of Astrophysical Turbulence; Wolfram Schmidt Book 2014 The Author(s) 2014 Astrophysical Turbulence.Astrophysical Turbu

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發(fā)表于 2025-3-21 19:48:09 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱Numerical Modelling of Astrophysical Turbulence
編輯Wolfram Schmidt
視頻videohttp://file.papertrans.cn/670/669138/669138.mp4
概述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 s
叢書(shū)名稱SpringerBriefs in Astronomy
圖書(shū)封面Titlebook: Numerical Modelling of Astrophysical Turbulence;  Wolfram Schmidt Book 2014 The Author(s) 2014 Astrophysical Turbulence.Astrophysical Turbu
描述.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..
出版日期Book 2014
關(guān)鍵詞Astrophysical Turbulence; Astrophysical Turbulence Basics; Compressible Turbulence; Computational Fluid
版次1
doihttps://doi.org/10.1007/978-3-319-01475-3
isbn_softcover978-3-319-01474-6
isbn_ebook978-3-319-01475-3Series ISSN 2191-9100 Series E-ISSN 2191-9119
issn_series 2191-9100
copyrightThe Author(s) 2014
The information of publication is updating

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Numerical Modelling of Astrophysical Turbulence978-3-319-01475-3Series ISSN 2191-9100 Series E-ISSN 2191-9119
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https://doi.org/10.1007/978-3-319-01475-3Astrophysical Turbulence; Astrophysical Turbulence Basics; Compressible Turbulence; Computational Fluid
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Turbulent Velocity Statistics,e in the highly compressible regime. If the forcing is strong enough to produced supersonic flow velocities, the dissipation of the kinetic energy rapidly heats the gas, which entails a continuously rising speed of sound. For this reason, supersonic turbulence in a steady state with constant mean Ma
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