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Magnetohydrodynamics. --- Magneto-hydrodynamics --- MHD (Physics) --- Fluid dynamics --- Plasma dynamics
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Magnetic fields influence many natural and man-made flows. They are routinely used in industry to heat, pump, stir and levitate liquid metals. There is the terrestrial magnetic field which is maintained by fluid motion in the earth's core, the solar magnetic field, which generates sunspots and solar flares, and the galactic field which influences the formation of stars. This is an introductory text on magnetohydrodynamics (MHD) - the study of the interaction of magnetic fields and conducting fluids. This book is intended to serve as an introductory text for advanced undergraduates and postgraduate students in physics, applied mathematics and engineering. The material in the text is heavily weighted towards incompressible flows and to terrestrial (as distinct from astrophysical) applications. The final sections of the text also contain an outline of the latest advances in the metallurgical applications of MHD and so are relevant to professional researchers in applied mathematics, engineering and metallurgy.
Fluid mechanics --- Magnetohydrodynamics --- Magnétohydrodynamique --- Magnetohydrodynamics. --- Magnétohydrodynamique --- Magneto-hydrodynamics --- MHD (Physics) --- Fluid dynamics --- Plasma dynamics
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This textbook provides a modern and accessible introduction to magnetohydrodynamics (MHD). It describes the two main applications of plasma physics, laboratory research on thermo-nuclear fusion energy and plasma astrophysics of the solar system, stars and accretion disks, from the single viewpoint of MHD. This approach provides effective methods and insights for the interpretation of plasma phenomena on virtually all scales, from the laboratory to the universe. It equips the reader with the necessary tools to understand the complexities of plasma dynamics in extended magnetic structures. The classical MHD model is developed in detail without omitting steps in the derivations and problems are included at the end of each chapter. This text is ideal for senior-level undergraduate and graduate courses in plasma physics and astrophysics.
Plasma physics --- Magnetohydrodynamics. --- Magnétohydrodynamique --- 537.84 --- 537.84 Magnetohydrodynamics --- Magnetohydrodynamics --- Magnétohydrodynamique --- Magneto-hydrodynamics --- MHD (Physics) --- Fluid dynamics --- Plasma dynamics
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"Studies based on the Rankine-Hugoniot relations have classified MHO shock waves as fast, switch-on, intermediate, switch-off, and slow. Any waves found in nature must also: (a) possess steady-state structures and (b) be stable in the presence of small-flow disturbances. In this monograph, Dr. Anderson examines these criteria in relation to plane shocks for which the collision frequency is large compared with cyclotron frequency. It contains a three-dimensional graphic representation of shock end states and presents an exact solution for the shock adiabatic curve in a convenient form."
Magnetohydrodynamics. --- Magneto-hydrodynamics --- MHD (Physics) --- Fluid dynamics --- Plasma dynamics --- Magnetohydrodynamic waves. --- Shock waves. --- PHYSICAL SCIENCES/General --- ENGINEERING/Mechanical Engineering
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Plasma physics --- Fluid mechanics --- Magnetohydrodynamics --- 533.9 --- #KVIV --- Magneto-hydrodynamics --- MHD (Physics) --- Fluid dynamics --- Plasma dynamics --- Magnetohydrodynamics. --- 533.9 Plasma physics
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533.9 --- Astrophysics --- Magnetohydrodynamics --- Magneto-hydrodynamics --- MHD (Physics) --- Fluid dynamics --- Plasma dynamics --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Plasma physics --- 533.9 Plasma physics --- Sun --- Sun. --- Solar system
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This book presents the collective drift and MHD-type modes in inhomogeneous plasmas from the point of view of two-fluid and kinetic theory. It emphasizes the description of the plasma rather than the geometry to present a more general approach to a large class of plasma problems. Starting with generalized fluid equations for low frequency phenomena, the author shows how drift waves and MHD-type modes can arise from the effects of inhomogeneities in the plasma. The kinetic description is then presented to reveal a host of phenomena ranging from vortex modes and finite Larmor radius effects to trapped and fast particle instabilities, transport, diffusion, and other advanced fluid effects.
Plasma dynamics --- Magnetohydrodynamics --- Plasmas, Dynamique des --- Magnétohydrodynamique --- Plasma dynamics. --- Magnetohydrodynamics. --- Magneto-hydrodynamics --- MHD (Physics) --- Fluid dynamics --- Snowplow effect --- Dynamics --- Plasma (Ionized gases) --- Magnétohydrodynamique
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Plasma (Ionized gases) --- Magnetohydrodynamics --- Plasma (Gaz ionisés) --- Magnétohydrodynamique --- Magnetohydrodynamics. --- Gaseous discharge --- Gaseous plasma --- Magnetoplasma --- Magneto-hydrodynamics --- MHD (Physics) --- Ionized gases --- Fluid dynamics --- Plasma dynamics
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-Magnetohydrodynamics --- -Cosmic plasmas --- Magneto-hydrodynamics --- MHD (Physics) --- Atmosphere, Upper --- Magnetohydrodynamics --- Magnetosphere --- Space plasmas --- Congresses. --- 52 --- Congresses --- Astronomie. Astrofysica. Ruimteonderzoek. Geodesie --- Atmosphere [Upper ] --- Aeronomy --- Atmosphere
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Generators [Magnetohydrodynamic ] --- MHD (Physics) --- MHD generators --- Magneto-hydrodynamics --- Magnetohydrodynamic generators --- Magnetohydrodynamica --- Magnetohydrodynamics --- Magnetohydrodynamique --- Electric power production - Magnetohydrodynamic generation. --- Electric power production --- Magnetohydrodynamic generators. --- Magnetohydrodynamics. --- Magnetohydrodynamic generation.
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