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Titlebook: An Introduction to Plasma Astrophysics and Magnetohydrodynamics; Marcel Goossens Book 2003 Springer Science+Business Media Dordrecht 2003

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发表于 2025-3-21 17:28:01 | 显示全部楼层 |阅读模式
期刊全称An Introduction to Plasma Astrophysics and Magnetohydrodynamics
影响因子2023Marcel Goossens
视频video
学科分类Astrophysics and Space Science Library
图书封面Titlebook: An Introduction to Plasma Astrophysics and Magnetohydrodynamics;  Marcel Goossens Book 2003 Springer Science+Business Media Dordrecht 2003
影响因子.Most of the visible matter in the universe exists in the plasma state. Plasmas are of major importance for space physics, solar physics, and astrophysics. On Earth they are essential for magnetic controlled thermonuclear fusion. ..This textbook collects lecture notes from a one-semester course taught at the K.U. Leuven to advanced undergraduate students in applied mathematics and physics. A particular strength of this book is that it provides a low threshold introduction to plasmas with an emphasis on first principles and fundamental concepts and properties. ..The discussion of plasma models is to a large extent limited to Magnetohydrodynamics (MHD) with its merits and limitations clearly explained. MHD provides the students on their first encounter with plasmas, with a powerful plasma model that they can link to familiar classic fluid dynamics. The solar wind is studied as an example of hydrodynamics and MHD at work in solar physics and astrophysics. .
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Franz Koenigsberger,Rolf Hackstein very short cyclotron time scale and the gyro-radius length scale. At the other end, it accurately describes the macroscopic behaviour of large astrophysical and fusion plasmas. The complexity arising from this wide range of plasma physics information makes it virtually impossible to solve the Boltz
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Introduction,re (almost) everywhere in the universe and to point out that they are extremely complicated physical systems fundamentally different from classic neutral gases, especially when there is a magnetic field present. The hope is that the reader is convinced that plasmas are exciting physical objects that
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Fluid equations for mass, momentum and energy, very short cyclotron time scale and the gyro-radius length scale. At the other end, it accurately describes the macroscopic behaviour of large astrophysical and fusion plasmas. The complexity arising from this wide range of plasma physics information makes it virtually impossible to solve the Boltz
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Basic plasma properties, range electromagnetic interaction between the charged particles. In this Chapter we shall study the two basic characteristics that are used in the definition of a plasma: quasi-neutrality and collective behaviour. We shall determine basic consequences arising from the long-range Coulomb interaction
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Fluid equations for mass, momentum and energy, plasmas are most accurately described by particle distribution functions in phase space. The spatial and temporal evolution of these distribution functions are governed by the Boltzmann equation (2.9). This is a partial differential equation in a 7-dimensional space. Chapman and Enskog were the fir
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Magnetohydrodynamics, Chapter do not form a closed set. The aim of this Chapter is to obtain closure. Let us recall that expressions for the anisotropic part of the stress tensor and for the flux of heat due to random motions are necessary but not sufficient for obtaining this goal. Inspection of the single-fluid equati
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