Ivan, L. (2014). A Fourth-Order Solution-Adaptive CENO Scheme for Space-Physics Flows on Three-Dimensional Multi-Block Cubed-Sphere Grids. Perimeter Institute. https://pirsa.org/14050051
MLA
Ivan, Lucian. A Fourth-Order Solution-Adaptive CENO Scheme for Space-Physics Flows on Three-Dimensional Multi-Block Cubed-Sphere Grids. Perimeter Institute, May. 07, 2014, https://pirsa.org/14050051
BibTex
@misc{ pirsa_PIRSA:14050051,
doi = {10.48660/14050051},
url = {https://pirsa.org/14050051},
author = {Ivan, Lucian},
keywords = {},
language = {en},
title = {A Fourth-Order Solution-Adaptive CENO Scheme for Space-Physics Flows on Three-Dimensional Multi-Block Cubed-Sphere Grids},
publisher = {Perimeter Institute},
year = {2014},
month = {may},
note = {PIRSA:14050051 see, \url{https://pirsa.org}}
}
Accurate efficient and scalable computational methods are highly desirable for large-scale scientific computing applications especially for problems exhibiting spatial and temporal multi-resolution scales non-trivial geometries and complex boundary conditions (BSc). For global magnetohydrodynamics (MHD) modelling of space-physics problemshigh-performance approaches could significantly reduce the grid requirements to achieve targeted solution accuracies thereby enabling more affordable yet accurate predictions of space-plasma flows. Key challenges encountered relate to providing solenoidal magnetic fields accurate discretizations on spherical domains capturing of MHD shocks and implementing accurate BCs. This talk gives an overview of a fourth-order finite-volume discretization procedure in combination with a parallel solution-adaptive algorithm for the computation of MHD space plasmas on cubed-sphere grids. Numerical results to demonstrate the accuracy and capability of the multidimensional high-order solution-adaptive cubed-sphere computational framework are presented.
