Solar Convection Simulations using a B-spline method
Thomas Hartlep, Nagi N. Mansour
TL;DR
This paper presents a novel B-spline spectral numerical code designed for simulating solar convection flows, enabling variable spatial resolution in all three dimensions to improve simulation accuracy.
Contribution
The development of a flexible B-spline spectral code that adapts spatial resolution in all directions for enhanced solar convection modeling.
Findings
Allows variable spatial resolution in all three coordinates
Improves accuracy of solar convection simulations
Provides a new tool for astrophysical fluid dynamics
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsPlant Water Relations and Carbon Dynamics · Fluid Dynamics and Turbulent Flows · Wind and Air Flow Studies