Impurities in a non-axisymmetric plasma: transport and effect on bootstrap current
Albert Moll\'en (1), Matt Landreman (2), H\r{a}kan M. Smith (3),, Stefanie Braun (3, 4), Per Helander (3) ((1) Department of Applied, Physics, Chalmers University of Technology, G\"oteborg, Sweden, (2) Institute, for Research in Electronics, Applied Physics

TL;DR
This paper uses a new kinetic solver to analyze impurity transport and its impact on bootstrap current in stellarator plasmas, revealing key scaling behaviors and effects of impurity content.
Contribution
It introduces the SFINCS code for detailed impurity transport calculations and compares results with theoretical asymptotes, highlighting new impurity transport scalings.
Findings
1/nu-scaling of inter-species radial transport at low collisionality
Radial electric field suppresses certain impurity transport scalings
Impurity content significantly affects bootstrap current and divertor strike points
Abstract
Impurities cause radiation losses and plasma dilution, and in stellarator plasmas the neoclassical ambipolar radial electric field is often unfavorable for avoiding strong impurity peaking. In this work we use a new continuum drift-kinetic solver, the SFINCS code (the Stellarator Fokker-Planck Iterative Neoclassical Conservative Solver) [M. Landreman et al., Phys. Plasmas 21 (2014) 042503] which employs the full linearized Fokker-Planck-Landau operator, to calculate neoclassical impurity transport coefficients for a Wendelstein 7-X (W7-X) magnetic configuration. We compare SFINCS calculations with theoretical asymptotes in the high collisionality limit. We observe and explain a 1/nu-scaling of the inter-species radial transport coefficient at low collisionality, arising due to the field term in the inter-species collision operator, and which is not found with simplified collision models…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
