Fluid simulations of plasma filaments in stellarator geometries with BSTING
B Shanahan, B Dudson, and P Hill

TL;DR
This paper introduces a fluid simulation framework for plasma filaments in stellarator geometries, utilizing advanced grid generation and coordinate schemes, and presents initial results on filament behavior in non-axisymmetric magnetic fields.
Contribution
The paper develops a 3D flux coordinate independent scheme within the BOUT++ framework for simulating plasma filaments in stellarator geometries, including new grid generation techniques.
Findings
Filaments propagate in a non-uniform toroidal manner.
Long connection lengths enable parallel gradients in the scrape-off-layer.
Filament velocity scales suggest inertial-limited propagation.
Abstract
Here we present first results simulating plasma filaments in non-axisymmetric geometries, using a fluid turbulence extension of the \boutxx~framework. This is made possible by the implementation of the Flux Coordinate Independent scheme for parallel derivatives, an extension of the metric tensor components which allows them to vary in three dimensions, and development of grid generation. Tests have been performed to confirm that the extension to three dimensional metric tensors does not compromise the accuracy and stability of the associated numerical operators. Recent changes to the FCI grid generator in \boutxx, including a curvilinear grid system which allows for potentially more efficient computation, are also presented. Initial simulations of seeded plasma filaments in a non-axisymmetric geometry are reported. We characterize filaments propagating in the closed-field-line region of…
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