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Identification of Magnetic Reconnection in Plasma Turbulence Using a Dual-branch Lightweight Hybrid Convolutional Neural Network

Authors: Y. Yin, S. Y. Huang, Q. Y. Xiong, H. Zhang, Z. G. Yuan, K. Jiang, H. H. Wu, H. W. Zhan, Y. T. Tang, H. Bai

Y. Yin et al 2026 The Astrophysical Journal Supplement Series 287 .

Caption: Figure 6.

The core architecture of the deep separable neural networks, consisting of a depth-wise convolution followed by a point-wise convolution.