pith. sign in

arxiv: 0712.0954 · v1 · submitted 2007-12-06 · 🌌 astro-ph

The Numerical Simulation of Turbulence

classification 🌌 astro-ph
keywords numericalbasicphysicalproblemsturbulenceapproachescommonlycomputational
0
0 comments X
read the original abstract

In this contribution, I give an overview of the various approaches toward the numerical modelling of turbulence, particularly, in the interstellar medium. The discussion is placed in a physical context, i. e. computational problems are motivated from basic physical considerations. Presenting selected examples for solutions to these problems, I introduce the basic ideas of the most commonly used numerical methods.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.