On the proper treatment of magnetic fluctuations in full-$f$ field-aligned turbulence codes
Kaiyu Zhang, Wladimir Zholobenko, Andreas Stegmeir, Konrad Eder, and, Frank Jenko

TL;DR
This paper addresses the inconsistency in full-$f$ plasma turbulence simulations caused by background magnetic components in magnetic fluctuations, proposing a dynamic filtering method to improve numerical accuracy in field-aligned codes.
Contribution
It introduces a novel dynamic filtering technique to accurately separate background magnetic fields from turbulent fluctuations in full-$f$ turbulence simulations.
Findings
The filtering method preserves turbulence fidelity in tokamak simulations.
It prevents spurious transport caused by improper background removal.
The approach is validated in both low and high confinement conditions.
Abstract
Plasma turbulence in the edge of magnetic confinement devices is customarily treated as full- due to large fluctuations. For computational efficiency, field-aligned coordinates are employed, separating the magnetic field into equilibrium and delta-f perturbations which are handled by the magnetic flutter operators. Evolving the full- pressure with delta- magnetic perturbations can cause inconsistency since the latter contain background components such as the Shafranov shift, which are actually parts of the equilibrium magnetic field. Such background components () contained in the magnetic perturbations undermine the field-aligned numerics when treated as flutter: errors arise if is not satisfied, with the perpendicular turbulence scale and the parallel grid distance . We find that the commonly used removal of…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies · Magnetic confinement fusion research
