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The Dynamic Structure of Coronal Hole Boundaries

  • Authors: V. Aslanyan, D. I. Pontin, R. B. Scott, A. K. Higginson, P. F. Wyper, S. K. Antiochos

V. Aslanyan et al 2022 The Astrophysical Journal 931 .

  • Provider: AAS Journals

Caption: Figure 1.

Vertical cut through the three-dimensional MHD simulation domain showing magnetic field structure. Outside the photosphere (gray), regions filled with open magnetic field lines are colored blue, closed regions colored red, and the border between them highlighted by the white line (not itself a field line). Sample field lines are indicated in blue and red respectively. The small isolated closed region in the top right is the pseudostreamer.

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