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Real-time solar coronal modelling

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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 regions for space weather.

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Fig. 1: Comparison between model and observations of the solar active region AR 11158.

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  1. Sydney Institute for Astronomy, School of Physics, The University of Sydney, New South Wales, Australia

    Michael S. Wheatland

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  1. Michael S. Wheatland
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Correspondence to Michael S. Wheatland.

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Wheatland, M.S. Real-time solar coronal modelling. Nat Astron 7, 1150–1151 (2023). https://doi.org/10.1038/s41550-023-02085-8

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