Real-time solar coronal modelling

Physics-informed neural networks allow the construction of state-of-the-art models of magnetic fields in active regions on the Sun in real time, enabling rapid investigation of the source

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support REFERENCES * Jarolim, R., Thalmann, J. K., Veronig, A. M. & Podladchikova, T. _Nat. Astron._ https://doi.org/10.1038/s41550-023-02030-9 (2023). Article  Google Scholar  *

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AFFILIATIONS * Sydney Institute for Astronomy, School of Physics, The University of Sydney, New South Wales, Australia Michael S. Wheatland Authors * Michael S. Wheatland View author

publications You can also search for this author inPubMed Google Scholar CORRESPONDING AUTHOR Correspondence to Michael S. Wheatland. ETHICS DECLARATIONS COMPETING INTERESTS The author

declares no competing interests. RIGHTS AND PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE Wheatland, M.S. Real-time solar coronal modelling. _Nat Astron_ 7,

1150–1151 (2023). https://doi.org/10.1038/s41550-023-02085-8 Download citation * Published: 17 October 2023 * Issue Date: October 2023 * DOI: https://doi.org/10.1038/s41550-023-02085-8 SHARE

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