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A Swin Transformer for Multiparameter Solar Wind Forecasting from MHD Simulations

  • Authors: Yiwan Deng, Yike Qiu, Zhou Chen, Kening Zhang, Tingfeng Xie, Jing-Song Wang

Yiwan Deng et al 2026 The Astrophysical Journal 1011 .

  • Provider: AAS Journals

Caption: Figure 10.

Comparison of the standard correlation coefficients CC (pink) and weighted correlation coefficients wCC (blue) for nine solar wind parameters at rolling steps 1, 5, and 9 on the test set. The CC is calculated between the rolling predictions at the near-Earth grid point (r ≈ 215 Rs) and hourly OMNI observations. The wCC is calculated between the predictions and the MHD true values in the two-dimensional spatial domain. Each step corresponds to a forecast advance of 24 hr.

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