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Numerical resistivity

Numerical resistivity is a problem in computer simulations of ideal magnetohydrodynamics (MHD). It is a form of numerical diffusion. In near-ideal… 
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Related topics

Related topics

3 relations
Computer simulationList of numerical analysis topicsNumerical diffusion

Papers overview

Semantic Scholar uses AI to extract papers important to this topic.
2018
2018
Can an interplanetary magnetic field reach the surface of Venus?
Abstract. We address the question of whether there is a possibility of an interplanetary magnetic field reaching Venus' surface… 
2016
2016
Length Scales and Turbulent Properties of Magnetic Fields in Simulated Galaxy Clusters
Additional physics beyond standard hydrodynamics is needed to fully model the intracluster medium (ICM); however, as we move to… 
2014
2014
Toward A Self Consistent MHD Model of Chromospheres and Winds From Late Type Evolved Stars
We present the first magnetohydrodynamic model of the stellar chromospheric heating and acceleration of the outer atmospheres of… 
Review
2010
Review
2010
We present a survey of magnetic reconnection at the dayside magnetopause using the Lyon
[1] We present a survey of magnetic reconnection at the dayside magnetopause using the Lyon‐Fedder‐Mobarry global magnetospheric… 
2007
2007
Fluxon modeling of low-beta plasmas
We have developed a new, quasi-Lagrangian approach for numerical modeling of magnetohydrodynamics in low to moderate b plasmas… 
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