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Neural network reconstruction of the DIII-D tokamak plasma boundary using a reduced set of diagnostics

Published online by Cambridge University Press:  26 January 2026

Maksim Stokolesov*
Affiliation:
Next Step Fusion, 33 Rue Du Puits Romain, Bertrange 8070, Luxembourg
Maxim Nurgaliev
Affiliation:
Next Step Fusion, 33 Rue Du Puits Romain, Bertrange 8070, Luxembourg
Ivan Kharitonov
Affiliation:
Next Step Fusion, 33 Rue Du Puits Romain, Bertrange 8070, Luxembourg
Evgeny Adishchev
Affiliation:
Next Step Fusion, 33 Rue Du Puits Romain, Bertrange 8070, Luxembourg
Dmitry Sorokin
Affiliation:
Next Step Fusion, 33 Rue Du Puits Romain, Bertrange 8070, Luxembourg
Randall Clark
Affiliation:
Center for Energy Research, University of California San Diego, La Jolla, CA 92122, USA
Dmitri Orlov
Affiliation:
Center for Energy Research, University of California San Diego, La Jolla, CA 92122, USA
*
Corresponding author: Maksim Stokolesov, stokolesov.ms@gmail.com

Abstract

This study investigates the feasibility of reconstructing the last closed flux surface in the DIII-D tokamak using neural network models trained on reduced input feature sets, addressing an ill-posed task. Two models are compared: one trained solely on coil currents and another incorporating coil currents, plasma current and loop voltage. The model trained exclusively on coil currents achieved a mean point displacement of $0.04$ m on a held-out test set, while the inclusion of plasma current and loop voltage reduced the error to $0.03$ m. This comparison highlights the trade-offs between input feature complexity and reconstruction accuracy, demonstrating the potential of machine learning algorithms to perform effectively in data-limited environments, such as those expected in fusion power plants due to diagnostic constraints imposed by the presence of blankets and shielding.

Information

Type
Letter
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2026. Published by Cambridge University Press
Figure 0

Table 1. Correspondence between models and the input feature sets they were trained on. Here, $k$ represents the magnetic coil index, and ${{N_{\text{coils}}}} = 20$ in this work for DIII-D.

Figure 1

Figure 1. Left: heatmap of the correlation matrix between dataset features (model inputs, left) and target plasma boundary points (model outputs, top). The left part of the matrix corresponds to the $R$ coordinates of the boundary points, the right part corresponds to the $Z$ coordinates. For clarity, each boundary point is labelled by its polar angle (in degrees) relative to the plasma centre and the positive direction of the $R$ axis. Right: poloidal cross-section of the DIII-D magnet system shown for geometric reference.

Figure 2

Figure 2. Centre plot: distribution of plasma states in the training dataset based on top and bottom triangularity. All states are divided into three main groups, producing 12 subgroups for cross-validation. At each cross-validation stage, the training set is composed of data from 11 groups, while the remaining group is used for testing. The left and right plots show examples of plasma shapes with ‘negative–positive’ and ‘negative–negative’ triangularity, respectively, illustrating the models’ accuracy on previously unseen cases (orange – true boundary, blue – model #1 reconstruction, green – model #2).

Figure 3

Table 2. Performance of the models during cross-validation. The metric values are averaged across cross-validation splits.

Figure 4

Figure 3. Dynamics of the MSE loss during training of the model #2 for the training set (blue) and the validation set (orange).

Figure 5

Figure 4. Probability density histograms of key plasma parameters in the training and test sets. The toroidal field is evaluated at the magnetic axis. Counts are normalised by the total number of samples and the bin width, yielding an estimate of the probability density function (PDF) and facilitating comparison between datasets of different sizes.

Figure 6

Table 3. Performance of the models on the test set.

Figure 7

Figure 5. Distribution of the $R^2$ metric for the $R$ and $Z$ coordinates of plasma boundary points for the model #2 on the test set. Plasma boundary points are labelled by their polar angle (in degrees) relative to the plasma centre and the positive direction of the $R$ axis.

Figure 8

Figure 6. Centre plot: distribution of the MXD metric across plasma states in the test subset (model #2). Examples of plasma shapes are shown for ‘positive–negative’ triangularity (left plot) and ‘positive–positive’ triangularity (right plot), with orange indicating the true boundary, blue – model #1 reconstruction, and green – model #2. These examples are taken from regions (highlighted in red) far from the majority of training samples (see figure 2) and represent challenging cases for the models (MXD values of $0.25$$0.3$ m).

Figure 9

Figure 7. Comparison of MXD (left) and MND (right) metric distributions for models #1 (blue) and #2 (green) on samples from the entire test subset. Histogram values are computed for individual samples. Vertical red lines indicate quantiles for model #2, with the top number representing the quantile and the bottom number showing the corresponding quantile value.