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 Series287.
Provider: AAS Journals
Caption: Figure 4.
The result of data augmentation: (a) the original image, (b) random rotation with angles in the range of (−15°, 15°), (c) random flipping, and (d) random noise.