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Unveiling the True Nature of Plasma Dynamics from the Reference Frame of a Superpenumbral Fibril

  • Authors: W. Bate, D. B. Jess, S. D. T. Grant, A. Hillier, S. J. Skirvin, T. Van Doorsselaere, S. Jafarzadeh, T. Wiegelmann, T. Duckenfield, C. Beck, T. Moore, M. Stangalini, P. H. Keys, D. J. Christian

W. Bate et al 2024 The Astrophysical Journal 970 .

  • Provider: AAS Journals

Caption: Figure 4.

The top panel shows the HMI SHARP 5961, used for the NLFFF extrapolation. This is shown with the associated CEA coordinates. The lower panel shows this same patch used as a mask on HMI data and the associated helioprojective coordinates. The magnetic field in the upper panel is calculated with respect to an observer directly above the sunspot center; in the lower panel it is with respect to the line of sight of SDO. Both magnetic field values are cropped at ±300 G for clarity.

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