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A Nonspherical Source Surface Model for the Solar Coronal Magnetic Field

  • Authors: Ziqi Wu, Jiansen He, Chuanpeng Hou, Tom Van Doorsselaere, Rui Zhuo, Tianhang Chen, Liping Yang, David Pontin, Daniel Verscharen, Fang Shen

Ziqi Wu et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 1.

The structure of the NSPF model. The model comprises three concentric layers: (1) a potential field layer; (2) a current sheet layer; (3) an interplanetary layer. The interface between the potential field and current sheet layers is the NSSS, while the interface between the current sheet and interplanetary layers is the exit sphere (located at 10 R⊙). Magnetic field lines and layer boundaries are labeled.

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