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Explainable AI for Solar Flare Prediction: Quantitative Magnetic Field Analysis of Model-focused Regions

  • Authors: Z. Zheng, Q. Hao, C. Li, P. F. Chen, J. R. Hu, M. D. Ding, C. Fang

Z. Zheng et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 4.

Schematic representation of the CNN model used in this work. Four-channel magnetic field images (BlosBrBp, and Bt) with an input size (4, 512, 512) are processed through convolutional and residual blocks, followed by global average pooling and sigmoid classification to predict the probability of flare occurrence within 24 hr. The final convolutional layer, which is used as the target layer for Grad-CAM, is highlighted.

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