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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 6.

Flux rope and associated current density distribution for AR 11429, derived from the CFIT N solution. (a) Dashed lines indicate the locations of vertical slices perpendicular to the main PIL considered for analysis. The lower boundary shows Bz(xy, 0) and the main PIL, similar to previous figures. (b) Current density in a vertical slice perpendicular to the upper section of the PIL (black dashed line in panel (a)). The field lines passing through the vertical slice are colored by ∣JCFIT(xyz)∣, sampled along the line. The normal current density in the slice, Jn, is positive for currents flowing in the direction of the normal vector to the plane. (c) Similar to panel (b) but for a vertical slice perpendicular to the lower section of the PIL (magenta dashed line in panel (a)).

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