ON THE CYLINDRICAL GRAD-SHAFRANOV EQUATION

摘要

The goal of this paper is to pay 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 the astrophysical jets we observe. In particular, it allows us to describe the central (and, hence, the most energetic) part of the flow.