Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 .

  • Provider: AAS Journals

Caption: Figure 1.

Snapshots of the current density at two different times in the simulation. (a) Current density at t = 34 ﹩{{\rm{\Omega }}}_{i}^{-1}﹩, where the CS is relatively clear, marked by the red circle. (b) Current density at t = 100 ﹩{{\rm{\Omega }}}_{i}^{-1}﹩, where the CS is relatively indistinct.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse