On the Cylindrical Grad-Shafranov Equation
Astrophysics
2009-06-23 v1
Abstract
The goal of this presentation is in paying attention to the 1D cylindrical version of the Grad-Shafranov (GS) equation. In our opinion, this approach is more rich than classical self-similar ones, and more suitable for astrophysical jets we observe. In particular, it allows us describing the central (and, hence, the most energetic) part of the flow.
Cite
@article{arxiv.0802.0142,
title = {On the Cylindrical Grad-Shafranov Equation},
author = {V. S. Beskin and E. E. Nokhrina},
journal= {arXiv preprint arXiv:0802.0142},
year = {2009}
}
Comments
In proceedings of High Energy Phenomena in Relativistic Outflows, Dublin, Ireland