Global gyrokinetic simulations of ASDEX Upgrade up to the transport time-scale with GENE-Tango
A. Di Siena, A. Banon Navarro, T. Luda, G. Merlo, M. Bergmann, L., Leppin, T. Goerler, J. B. Parker, L. LoDestro, J. Hittinger, B. Dorland, G., Hammett, F. Jenko, the ASDEX Upgrade Team, and the EUROfusion MST1 Team

TL;DR
This paper introduces GENE-Tango, a coupled gyrokinetic and transport solver, enabling high-fidelity, long-time plasma profile simulations that incorporate complex physics and significantly reduce computational costs, advancing fusion research.
Contribution
The paper presents the first coupling of GENE with Tango, allowing accurate transport-scale simulations with kinetic electrons, electromagnetic effects, and realistic geometries, overcoming previous limitations.
Findings
GENE-Tango accurately reproduces ion temperature peaking in ASDEX Upgrade discharges.
Electromagnetic effects of submarginal MHD instability influence ion temperature profiles.
Expected speedup for ITER scenarios exceeds two orders of magnitude.
Abstract
An accurate description of turbulence up to the transport time scale is essential for predicting core plasma profiles and enabling reliable calculations for designing advanced scenarios and future devices. Here, we exploit the gap separation between turbulence and transport time scales and couple the global gyrokinetic code GENE to the transport-solver Tango, including kinetic electrons, collisions, realistic geometries, toroidal rotation and electromagnetic effects for the first time. This approach overcomes gyrokinetic codes' limitations and enables high-fidelity profile calculations in experimentally relevant plasma conditions, significantly reducing the computational cost. We present numerical results of GENE-Tango for two ASDEX Upgrade discharges, one of which exhibits a pronounced peaking of the ion temperature profile not reproduced by TGLF-ASTRA. We show that GENE-Tango can…
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.
Taxonomy
TopicsMagnetic confinement fusion research · Ionosphere and magnetosphere dynamics
