Solar Convection Simulations using a B-spline method

Details Solar Convection Simulations using a B-spline method Solar Convection Simulations using a B-spline method

2008-05-05

arxiv.org/abs/0805.0571v1

Annual Research Briefs 2004, Center for Turbulence Research, Stanford University / NASA Ames Research Center, pp. 379-384

Astronomy and Astrophysics

Astrophysics

6 pages

Scientific paper

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.

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