What is it about?
The atmosphere of our Sun is populated by solar arcs. We propose a filament-based model of these arcs that allows us to recreate sun-like images. We also propose a pipeline to process magnetic flux surface data for our algorithm and apply it on NASA observatory data.
Photo by Arnaud Mariat on Unsplash
Why is it important?
Successfully modeling natural phenomena deepens our understanding of the underlying processes. It also allows the free generation of new data. The physics of the solar atmosphere is a great challenge to astrophysics and solar activity also affects our earth. This paper further lights the path in the understanding of the solar atmosphere.
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This page is a summary of: Filament based plasma, ACM Transactions on Graphics, July 2022, ACM (Association for Computing Machinery), DOI: 10.1145/3528223.3530102.
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