Solar Convection Simulations using a B-spline method

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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.
6 pages

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/160338

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0805.0571
 http://arxiv.org/abs/0805.0571
 Annual Research Briefs 2004, Center for Turbulence Research, Stanford University / NASA Ames Research Center, pp. 379-384

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arXiv