Historical perspective on astrophysical MHD simulations
Instrumentation and Methods for Astrophysics
2015-05-20 v1
Abstract
This contribution contains the introductory remarks that I presented at IAU Symposium 270 on ``Computational Star Formation" held in Barcelona, Spain, May 31 -- June 4, 2010. I discuss the historical development of numerical MHD methods in astrophysics from a personal perspective. The recent advent of robust, higher order-accurate MHD algorithms and adaptive mesh refinement numerical simulations promises to greatly improve our understanding of the role of magnetic fields in star formation.
Cite
@article{arxiv.1011.4625,
title = {Historical perspective on astrophysical MHD simulations},
author = {Michael L. Norman},
journal= {arXiv preprint arXiv:1011.4625},
year = {2015}
}
Comments
11 pages, 5 figures, in "Computational Star Formation" held in Barcelona, Spain, May 31 - June 4, 2010", Eds. J. Alves, B. G. Elmegreen, J. M. Girart, V. Trimble