Paley–Zygmund inequality: Difference between revisions

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'''Computational magnetohydrodynamics (CMHD)''' is a rapidly developing branch of [[magnetohydrodynamics]] that uses [[numerical method]]s and algorithms to solve and analyze problems that involve electrically conducting fluids. Most of the methods used in CMHD are borrowed from the well established techniques employed in [[Computational fluid dynamics]]. The complexity mainly arises due to the presence of a [[magnetic field]] and its coupling with the fluid. One of the important issues is to numerically maintain the <math> \nabla \cdot {\mathbf B} = 0</math> (conservation of magnetic flux) condition, from [[Maxwell's equations]], to avoid any unphysical effects.
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==See also==
* [[Magnetohydrodynamic turbulence]]
* [[Magnetic flow meter]]
 
==References==
* Brio, M., Wu, C. C.(1988), "An upwind differencing scheme for the equations of ideal magnetohydrodynamics", ''Journal of Computational Physics'', '''75''', 400&ndash;422.
* Henri-Marie Damevin and Klaus A. Hoffmann(2002), "Development of a Runge-Kutta Scheme with TVD for Magnetogasdynamics", ''Journal of Spacecraft and Rockets'', '''34''',No.4, 624&ndash;632.
* Robert W. MacCormack(1999), "An upwind conservation form method for ideal magnetohydrodynamics equations", ''AIAA-99-3609''.
* Robert W. MacCormack(2001), "A conservation form method for magneto-fluid dynamics", ''AIAA-2001-0195''.
 
==Further reading==
* Toro, E. F. (1999), ''Riemann Solvers and Numerical Methods for Fluid Dynamics'', Springer-Verlag.
==External links==
[http://www.ncbi.nlm.nih.gov/pmc/articles/PMC392293/ NCBI]
{{fluiddynamics-stub}}
 
[[Category:Numerical analysis]]

Latest revision as of 14:22, 25 September 2014

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