Simulation and Visualisation of Astrophysical Plasmas with Smoothed Particle Magnetohydrodynamics

Details Simulation and Visualisation of Astrophysical Plasmas with Smoothed Particle Magnetohydrodynamics Simulation and Visualisation of Astrophysical Plasmas with Smoothed Particle Magnetohydrodynamics

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010phdt.......101t&link_type=abstract

ProQuest Dissertations And Theses; Thesis (M.Sc.)--Memorial University of Newfoundland (Canada), 2010.; Publication Number: AAT

Computer Science

Scientific paper

A numerical implementation of the equations of magnetohydrodynamics has been developed using the Smoothed Particle Hydrodynamics (SPH) method. Self gravitational forces have been included using the Barnes-Hut octree algorithm. A nearest neighbour search algorithm has been devised which links adjacent, spatially exclusive nodes from a spatial decomposition tree to create a mesh facilitating efficient searching. Visualisations of SPH fluids were created using Delaunay triangulation with particles serving as triangle vertices.

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