On the Cylindrical Grad-Shafranov Equation
V. S. Beskin, E. E. Nokhrina
TL;DR
This paper explores the 1D cylindrical Grad-Shafranov equation, proposing it as a richer and more suitable model than classical self-similar approaches for describing the central regions of astrophysical jets.
Contribution
It introduces a cylindrical 1D version of the Grad-Shafranov equation, emphasizing its advantages for modeling energetic jet cores over traditional methods.
Findings
Provides a new framework for jet modeling
Highlights the equation's suitability for energetic regions
Suggests improved descriptions of astrophysical jets
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.
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