Reconstructions of electron-temperature profiles from EUROfusion pedestal database using turbulence models and machine learning

Journal of Plasma Physics. 2025;91(6):E155.

Authors:

L.-P. Turica, A.R. Field, A.A. Schekochihin, L. Frassinetti, JET Contributors, and the EUROfusion Tokamak Exploitation Team

Abstract:

This study makes use of plasma-profile data from the EUROfusion pedestal database (Frassinetti et al. 2020 Nucl. Fusion vol. 61, p. 016001), focusing on the electron-temperature and electron-density profiles in the edge region of H-mode ELMy JET ITER-Like-Wall (ILW) pulses. We make systematic predictions of the electron-temperature pedestal, taking engineering parameters of the plasma pulses and the density profiles as inputs. We first present a machine-learning (ML) algorithm which, given more inputs than theory-based modelling, is able to reconstruct unseen temperature profiles within 20 % of the experimental values. We find a hierarchy of the most consequential engineering parameters for such predictions. This result confirms the conceptual possibility of accurate data-driven prediction. Next, taking a simple theoretical approach that assumes a definite local relationship between the electron-density (𝑅/𝐿𝑛𝑒) and electron-temperature (𝑅/𝐿𝑇𝑒) gradients, we find that a range of power-law scalings 𝑅/𝐿𝑇𝑒 =𝐴⁒(𝑅/𝐿𝑛𝑒)𝛼 with 𝛼 β‰ˆ0.4 correctly capture the behaviour of the electron-temperature in the steep-gradient region. Fitting 𝐴 and 𝛼 independently for each pedestal reveals a clear one-to-one correlation, suggesting an underlying constraint in pedestal physics. The measured πœ‚π‘’ =𝐿𝑛𝑒/𝐿𝑇𝑒 values across the pedestal exhibit a wide distribution, significantly exceeding the slab-ETG linear stability threshold, implying either a non-linear threshold shift or a measurably supercritical saturated turbulent state. Finally, we fit parameters for scalings that relate the turbulent heat flux to the gradients 𝑅/𝐿𝑇𝑒 and 𝑅/𝐿𝑛𝑒, similarly to models extracted from gyrokinetic simulations. The inclusion of more experimental parameters is necessary for such models to match the accuracy of our ML results.

Finding Local Parallel Electric Fields in Magnetotail Reconnection Using a Two-Spacecraft Method

(2025)

Authors:

Jack White, Yuri V Khotyaintsev, Cecilia Norgren, Daniel Bruce Graham, Louis Richard

Statistical Study of Betatron and Fermi Electron Acceleration at Dipolarization Fronts

(2025)

Authors:

Apostolos Kolokotronis, Daniel Bruce Graham, Yuri V Khotyaintsev, Cecilia Norgren, Konrad Steinvall, Louis Richard

Orbital classification in rotating bar potentials using an empirical proxy of the second integral of motion

(2025)

Authors:

Tian-ye Xia, Juntai Shen, John Magorrian, Yu-jing Qin

Cosmic-ray transport in inhomogeneous media

Monthly Notices of the Royal Astronomical Society Oxford University Press 545:2 (2025) staf2108

Authors:

Robert J Ewart, Patrick Reichherzer, Shuzhe Ren, Stephen Majeski, Francesco Mori, Michael L Nastac, Archie FA Bott, Matthew W Kunz, Alexander A Schekochihin

Abstract:

A theory of cosmic-ray transport in multiphase diffusive media is developed, with the specific application to cases in which the cosmic-ray diffusion coefficient has large spatial fluctuations that may be inherently multiscale. We demonstrate that the resulting transport of cosmic rays is diffusive in the long-time limit, with an average diffusion coefficient equal to the harmonic mean of the spatially varying diffusion coefficient. Thus, cosmic-ray transport is dominated by areas of low diffusion even if these areas occupy a relatively small, but not infinitesimal, fraction of the volume. On intermediate time-scales, the cosmic rays experience transient effective subdiffusion, as a result of low-diffusion regions interrupting long flights through high-diffusion regions. In the simplified case of a two-phase medium, we show that the extent and extremity of the subdiffusivity of cosmic-ray transport is controlled by the spectral exponent of the distribution of patch sizes of each of the phases. We finally show that, despite strongly influencing the confinement times, the multiphase medium is only capable of altering the energy dependence of cosmic-ray transport when there is a moderate (but not excessive) level of perpendicular diffusion across magnetic-field lines.