Solar Convection Simulations using a B-spline method
Astrophysics
2008-05-06 v1
Abstract
This report outlines the development of a B-spline--spectral numerical code for the simulation of convection flows. It allows changing the spatial resolution in all three coordinates as a function of depth, which is especially advantageous for simulations of solar convection.
Keywords
Cite
@article{arxiv.0805.0571,
title = {Solar Convection Simulations using a B-spline method},
author = {Thomas Hartlep and Nagi N. Mansour},
journal= {arXiv preprint arXiv:0805.0571},
year = {2008}
}
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6 pages