297 citations · 1.4k across the 27 of their papers we have counts for
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Anisotropy of third-order structure functions in MHD turbulence
Andrea Verdini, Roland Grappin, Petr Hellinger +2
The measure of the third-order structure function, Y, is employed in the solar wind to compute the cascade rate of turbulence. In the absence of a mean field B0=0, Y is expected to…
Fourth Order Accurate Finite Volume CWENO Scheme For Astrophysical MHD Problems
Prabal Singh Verma, Jean-Mathieu Teissier, Oliver Henze +1
In this work, a simple fourth-order accurate finite volume semi-discrete scheme is introduced to solve astrophysical magnetohydrodynamics (MHD) problems on Cartesian meshes. Hydrod…
Higher Order Central Schemes for Multi-dimensional Hyperbolic Problems
Prabal Singh Verma, Wolf-Christian Müller
Different ways of implementing dimension-by-dimension CWENO reconstruction are discussed and the most efficient method is applied to develop a fourth order central scheme for multi…