«
»

Filament Based Plasma

Marcel Padilla, Oliver Gross, Felix Knoppel, Albert Chern, Ulrich Pinkall, Peter Schroder

Simulation of stellar atmospheres, such as that of our own sun, is a common task in CGI for scientific visualization, movies and games. A fibrous volumetric texture is a visually dominant feature of the solar corona—the plasma that extends from the solar surface into space. These coronal fibers can be modeled as magnetic filaments whose shape is governed by the magnetohydrostatic equation. The magnetic filaments provide a Lagrangian curve representation and their initial configuration can be prescribed by an artist or generated from magnetic flux given as a scalar texture on the sun’s surface. Subsequently the shape of the filaments is determined based on a variational formulation. The output is a visual rendering of the whole sun. We demonstrate the fidelity of our method by comparing the resulting renderings with actual images of our sun’s corona.

Filament Based Plasma

Posted by christopherbatty on May 9th, 2022 Posted in Uncategorized
(Comments are closed)