EFIT-Prime: Probabilistic and physics-constrained reduced-order neural network model for equilibrium reconstruction in DIII-D

S. Madireddy, C. Akçay, S. E. Kruger, T. Bechtel Amara, X. Sun, J. McClenaghan, J. Koo, A. Samaddar, Y. Liu, P. Balaprakash, L. L. Lao

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Abstract

We introduce EFIT-Prime, a novel machine learning surrogate model for EFIT (Equilibrium FIT) that integrates probabilistic and physics-informed methodologies to overcome typical limitations associated with deterministic and ad hoc neural network architectures. EFIT-Prime utilizes a neural architecture search-based deep ensemble for robust uncertainty quantification, providing scalable and efficient neural architectures that comprehensively quantify both data and model uncertainties. Physically informed by the Grad-Shafranov equation, EFIT-Prime applies a constraint on the current density J tor and a smoothness constraint on the first derivative of the poloidal flux, ensuring physically plausible solutions. Furthermore, the spatial location of the diagnostics is explicitly incorporated in the inputs to account for their spatial correlation. Extensive evaluations demonstrate EFIT-Prime's accuracy and robustness across diverse scenarios, most notably showing good generalization on negative-triangularity discharges that were excluded from training. Timing studies indicate an ensemble inference time of 15 ms for predicting a new equilibrium, offering the possibility of plasma control in real-time, if the model is optimized for speed.

Original languageEnglish
Article number092505
JournalPhysics of Plasmas
Volume31
Issue number9
DOIs
StatePublished - Sep 1 2024

Funding

This work is supported by the U.S. Department of Energy, Office of Fusion Energy Science (Award Nos. DE-AC02-06CH11357, DE-SC0021203, DE-FG02-95ER54309, and DE-SC0021380). The authors acknowledge the computational resources of the Argonne Leadership Computing Facility, which is a DOE Office of Science User Facility supported under the contract (No. DE-AC02-06CH11357), and Laboratory Computing Resource Center (LCRC) at the Argonne National Laboratory. The data used in this work are based upon work supported by the U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences, using the DIII-D National Fusion Facility, a DOE Office of Science user facility (Award(s) No. DE-FC02-04ER54698).

FundersFunder number
U.S. Department of Energy
Argonne National Laboratory
Office of Science
Laboratory Computing Resource Center
Fusion Energy SciencesDE-AC02-06CH11357, DE-SC0021380, DE-FC02-04ER54698, DE-SC0021203, DE-FG02-95ER54309

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