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Validating Coronal Magnetic Field Models Using Gaussian Separation

  • Authors: Abhinav G. Iyer, Michael S. Wheatland, Brian T. Welsch, Yang Liu, S.A. Gilchrist

Abhinav G. Iyer et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 8.

The NLFFF model for AR 11429 on 2012 March 6 23:36 UT using the optimization method. The background color denotes the Bz component at the photosphere. The green Bz = 0 contours indicate the main PILs. The field lines are colored by the magnitude of the current density ∣J∣, sampled along the line.

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