29 June 2026 to 3 July 2026
EICC, Edinburgh
Europe/London timezone

Extending the GRAY beam-tracer beyond the standard electron cyclotron heating modelling

Not scheduled
20m
EICC, Edinburgh

EICC, Edinburgh

150 Morrison St, Edinburgh EH3 8EE
Poster Presentation Scenario Development, Heating and Current Drive (MCF)

Description

Electron Cyclotron (EC) waves are playing an increasingly important role in the operation of next-generation fusion devices: Electron Cyclotron Resonant Heating (ECRH), will be the main plasma heating mechanism, and Electron Cyclotron Current Drive (ECCD) will be fundamental in controlling instabilities like sawteeth and Neoclassical Tearing Modes (NTM) [1]; in superconducting devices, EC waves are also becoming an essential tool to assist the ohmic breakdown in the start-up phase [2]; finally, the interaction between EC waves and runaway electrons is being investigated as a new promising channel for exploring runaway dynamics [3].

GRAY [4] is a well-established beam-tracing code and a valuable tool for modeling EC waves, whose use has so far been mostly limited to predictive modeling of standard ECRH scenarios. More recently, efforts have been made to extend the applicability of GRAY across several additional fronts.

We have designed and implemented robust algorithms for processing the inputs and improved the reliability of the simulation to enable realtime applications. The wave absorption model has been extended to also cover the conditions relevant for studying runaways-driven instabilities (n∥ > 1, high-energy anisotropic distribution). A new method, exploiting the algebraic properties of the dielectric tensor, has been developed to simultaneously compute all roots of the relativistic dispersion relation, including Electron Bernstein Waves (EBW). This solves numerical stability issues of the standard method and also enables the detection of mode conversion events, potentially unlocking new applications such as giving a first-order estimation of the conversion efficiency in the O-X-B heating scheme [5].

[1] M. Kong et al, Plasma Phys. Control. Fusion 64 044008 (2022)
[2] Yong-Su Na et al, Nucl. Fusion 65 093001 (2025)
[3] W. Bin et al, Physical Review Letters 129 045002 (2022)
[4] D. Farina, Fusion Science and Technology 52 154–160 (2007)
[5] H. P. Laqua, Plasma Phys. Control. Fusion 49 R1 (2007)

Author

Michele Guerini Rocco (Department of Physics, University of Milano-Bicocca, Milan, Italy)

Co-authors

Dr Lorenzo Figini (Institute for Plasma Science and Technology, National Research Council, Milan, Italy) Dr William Bin (institute for plasma science and technology, national research council, milan, italy) Dr Carmine Castaldo (Consorzio RFX, Padua, Italy) Dr Paolo Buratti (IAPS - INAF Institute for Space Astrophysics and Planetology, Rome, Italy - ENEA, Fusion and Nuclear Safety Department, Frascati, Rome, Italy) Dr Alessandro Cardinali (CNR, Institute for Complex Systems, Polytechnic University of Turin, Turin, Italy) Dr Francesco Napoli (ENEA, Fusion and Nuclear Safety Department, Frascati, Rome, Italy)

Presentation materials