Solar Convection Simulations using a B-spline method

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dc.creatorHartlep, Thomas
dc.creatorMansour, Nagi N.
dc.date2008-05-05
dc.date.accessioned2026-07-07T09:37:05Z
dc.date.available2026-07-07T09:37:05Z
dc.descriptionThis 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.
dc.description6 pages
dc.identifierhttps://arxiv.org/abs/0805.0571
dc.identifierhttp://arxiv.org/abs/0805.0571
dc.identifierAnnual Research Briefs 2004, Center for Turbulence Research, Stanford University / NASA Ames Research Center, pp. 379-384
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/160338
dc.subjectAstrophysics
dc.titleSolar Convection Simulations using a B-spline method
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