Lectures In Magnetohydrodynamics
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Author | : Dalton D. Schnack |
Publisher | : Springer Science & Business Media |
Total Pages | : 317 |
Release | : 2009-08-26 |
Genre | : Science |
ISBN | : 3642006876 |
Magnetohydrodynamics, or MHD, is a theoretical way of describing the statics and dynamics of electrically conducting uids. The most important of these uids occurring in both nature and the laboratory are ionized gases, called plasmas. These have the simultaneous properties of conducting electricity and being electrically charge neutral on almost all length scales. The study of these gases is called plasma physics. MHD is the poor cousin of plasma physics. It is the simplest theory of plasma dynamics. In most introductory courses, it is usually afforded a short chapter or lecture at most: Alfven ́ waves, the kink mode, and that is it. (Now, on to Landau damping!) In advanced plasma courses, such as those dealing with waves or kinetic theory, it is given an even more cursory treatment, a brief mention on the way to things more profound and interesting. (It is just MHD! Besides, real plasma phy- cists do kinetic theory!) Nonetheless, MHD is an indispensable tool in all applications of plasma physics.
Author | : Dalton D. Schnack |
Publisher | : Springer |
Total Pages | : 317 |
Release | : 2009-08-11 |
Genre | : Science |
ISBN | : 3642006884 |
Magnetohydrodynamics, or MHD, is a theoretical way of describing the statics and dynamics of electrically conducting uids. The most important of these uids occurring in both nature and the laboratory are ionized gases, called plasmas. These have the simultaneous properties of conducting electricity and being electrically charge neutral on almost all length scales. The study of these gases is called plasma physics. MHD is the poor cousin of plasma physics. It is the simplest theory of plasma dynamics. In most introductory courses, it is usually afforded a short chapter or lecture at most: Alfven ́ waves, the kink mode, and that is it. (Now, on to Landau damping!) In advanced plasma courses, such as those dealing with waves or kinetic theory, it is given an even more cursory treatment, a brief mention on the way to things more profound and interesting. (It is just MHD! Besides, real plasma phy- cists do kinetic theory!) Nonetheless, MHD is an indispensable tool in all applications of plasma physics.
Author | : Hannes Alfvén |
Publisher | : |
Total Pages | : 248 |
Release | : 1958 |
Genre | : Cosmic rays |
ISBN | : |
Author | : Hartmut Zohm |
Publisher | : John Wiley & Sons |
Total Pages | : 254 |
Release | : 2015-02-09 |
Genre | : Science |
ISBN | : 3527412328 |
This book bridges the gap between general plasma physics lectures and the real world problems in MHD stability. In order to support the understanding of concepts and their implication, it refers to real world problems such as toroidal mode coupling or nonlinear evolution in a conceptual and phenomenological approach. Detailed mathematical treatment will involve classical linear stability analysis and an outline of more recent concepts such as the ballooning formalism. The book is based on lectures that the author has given to Master and PhD students in Fusion Plasma Physics. Due its strong link to experimental results in MHD instabilities, the book is also of use to senior researchers in the field, i.e. experimental physicists and engineers in fusion reactor science. The volume is organized in three parts. It starts with an introduction to the MHD equations, a section on toroidal equilibrium (tokamak and stellarator), and on linear stability analysis. Starting from there, the ideal MHD stability of the tokamak configuration will be treated in the second part which is subdivided into current driven and pressure driven MHD. This includes many examples with reference to experimental results for important MHD instabilities such as kinks and their transformation to RWMs, infernal modes, peeling modes, ballooning modes and their relation to ELMs. Finally the coverage is completed by a chapter on resistive stability explaining reconnection and island formation. Again, examples from recent tokamak MHD such as sawteeth, CTMs, NTMs and their relation to disruptions are extensively discussed.
Author | : André Lichnerowicz |
Publisher | : |
Total Pages | : 216 |
Release | : 1967 |
Genre | : Fluid dynamics |
ISBN | : |
Author | : D. A. Gurnett |
Publisher | : Cambridge University Press |
Total Pages | : 468 |
Release | : 2005-01-06 |
Genre | : Science |
ISBN | : 9780521364836 |
Advanced undergraduate/beginning graduate text on space and laboratory plasma physics.
Author | : R.V. Polovin |
Publisher | : Springer |
Total Pages | : 360 |
Release | : 1990-01-31 |
Genre | : Science |
ISBN | : |
A text for teachers and students in experimental physics and research engineering, introducing the ideas of magnetohydrodynamics (MHD), showing the methods used in MHD, and preparing students for reading the original literature. Based on the mathematical study of simplified models. Annotation copyri
Author | : Roman Jackiw |
Publisher | : Springer Science & Business Media |
Total Pages | : 148 |
Release | : 2002-05-17 |
Genre | : Science |
ISBN | : 9780387954226 |
Explains the motivation and reviewing the classical theory in a new form; Discusses conservation laws and Euler equations; For one-dimensional cases, the models presented are completely integrable
Author | : Jonathan Braithwaite |
Publisher | : Morgan & Claypool Publishers |
Total Pages | : 195 |
Release | : 2018-01-09 |
Genre | : Science |
ISBN | : 1681745984 |
The book is an introduction to the subject of fluid mechanics, essential for students and researchers in many branches of science. It illustrates its fundamental principles with a variety of examples drawn mainly from astrophysics and geophysics as well as from everyday experience. Prior familiarity with basic thermodynamics and vector calculus is assumed.
Author | : Hans Goedbloed |
Publisher | : Cambridge University Press |
Total Pages | : 995 |
Release | : 2019-01-31 |
Genre | : Science |
ISBN | : 110857758X |
With ninety per cent of visible matter in the universe existing in the plasma state, an understanding of magnetohydrodynamics is essential for anyone looking to understand solar and astrophysical processes, from stars to accretion discs and galaxies; as well as laboratory applications focused on harnessing controlled fusion energy. This introduction to magnetohydrodynamics brings together the theory of plasma behavior with advanced topics including the applications of plasma physics to thermonuclear fusion and plasma- astrophysics. Topics covered include streaming and toroidal plasmas, nonlinear dynamics, modern computational techniques, incompressible plasma turbulence and extreme transonic and relativistic plasma flows. The numerical techniques needed to apply magnetohydrodynamics are explained, allowing the reader to move from theory to application and exploit the latest algorithmic advances. Bringing together two previous volumes: Principles of Magnetohydrodynamics and Advanced Magnetohydrodynamics, and completely updated with new examples, insights and applications, this volume constitutes a comprehensive reference for students and researchers interested in plasma physics, astrophysics and thermonuclear fusion.