Solar Convection Simulations using a B-spline method
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🌌 astro-ph
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convectionsimulationssolaradvantageousallowsb-splineb-spline--spectralchanging
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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.
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