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2014
Comprehensive, self-contained, and clearly written, this successor to Ideal Magnetohydrodynamics (1987) describes the macroscopic equilibrium and stability of high temperature plasmas - the basic fuel for the development of fusion power. Now fully updated, this book discusses the underlying physical assumptions for three basic MHD models: ideal ...
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Comprehensive, self-contained, and clearly written, this successor to Ideal Magnetohydrodynamics (1987) describes the macroscopic equilibrium and stability of high temperature plasmas - the basic fuel for the development of fusion power. Now fully updated, this book discusses the underlying physical assumptions for three basic MHD models: ideal ...
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2004
The ideal MHD equations The dynamics of magnetically confined plasmas, as exploited in laboratory nuclear fusion research and observed in astrophysical systems, is essentially of a macroscopic nature so that it can be studied in the fluid (MHD) model introduced in Chapter 2.
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The ideal MHD equations The dynamics of magnetically confined plasmas, as exploited in laboratory nuclear fusion research and observed in astrophysical systems, is essentially of a macroscopic nature so that it can be studied in the fluid (MHD) model introduced in Chapter 2.
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Liouville-type theorems for the 3D stationary Navier-Stokes, MHD and Hall-MHD equations
Journal of Mathematical Analysis and Applications, 2020Baoquan Yuan
exaly
MHD flow in liquid metal blankets: Major design issues, MHD guidelines and numerical analysis
Fusion Engineering and Design, 2021Leo Bühler +2 more
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SLAU2-MHD for Low Mach Magnetohydrodynamics (MHD) Simulations
AIAA AVIATION 2021 FORUM, 2021Tomohiro Mamashita +2 more
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Resonant MHD Waves in the Solar Atmosphere
Space Science Reviews, 2010Maarcel Goossens +2 more
exaly
Theoretical and experimental study of MHD (magnetohydrodynamic) micropump
Sensors and Actuators A: Physical, 2000Jaesung Jang, Seung S Lee
exaly
The MHD equations have served plasma physicists, space physicists and astrophysicists very well for the past several decades. Even so, one comes to the realization that the MHD equations are only an approximation that applies to systems where the collision rate between charged particles is fast enough to rapidly restore isotropy in the pressure tensor.
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