On the Cylindrical Grad-Shafranov Equation
arXiv:0802.0142 · doi:10.1142/S0218271808013352
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.
In proceedings of High Energy Phenomena in Relativistic Outflows, Dublin, Ireland
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