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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 5.

Comparison between the modeled IMF and PSP’s in situ measurements. (a) NSPF models vs. observations. (b) PFSS+PFCS models vs. observations. (c) PFSS models vs. observations. In each panel, the black solid line denotes the observed IMF, while the colored dashed lines represent the modeled IMF obtained from models with different (initial) source surface heights, as indicated in the legend. The text annotations indicate the performance metrics for each model.

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