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Real-time solar coronal modelling

Nature Astronomy volume 7, pages 1150–1151 (2023)Cite this article

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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.

References

  1. 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 

  2. Wiegelmann, T. & Sakurai, T. Living Rev. Sol. Phys. 18, 1 (2021).

    Article  ADS  Google Scholar 

  3. Wheatland, M. S. & Régnier, S. Astrophys. J. 700, L88 (2009).

    Article  ADS  Google Scholar 

  4. Karniadakis, G. E. et al. Nat. Rev. Phys. 3, 422–440 (2021).

    Article  Google Scholar 

  5. Baydin, A. G., Pearlmutter, B. A., Radul, A. A. & Siskind, J. M. J. Mach. Learn. Res. 18, 5595–5637 (2017).

    Google Scholar 

  6. Bobra, M. G. et al. Sol. Phys. 289, 3549–3578 (2014).

    Article  ADS  Google Scholar 

  7. Sun, X. et al. Astrophys. J. 748, 77 (2012).

    Article  ADS  Google Scholar 

  8. Cai, S. et al. Acta Mech.Sin. 37, 1727–1738 (2021).

    Article  ADS  MathSciNet  Google Scholar 

Download references

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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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