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Analysis of Solar Eruptions Deflecting in the Low Corona: Influence of the Magnetic Environment

  • Authors: Abril Sahade, Angelos Vourlidas, Cecilia Mac Cormack

Abril Sahade et al 2025 The Astrophysical Journal 978 .

  • Provider: AAS Journals

Caption: Figure 5.

Panel (a): 2D sketch representing the “topological” path (orange solid line). Magnetic closed-line apexes are denoted by the dark-edged rhomboids, and the starting point is denoted by the red cross. Panel (b): sketch of the 3D scenario. Only magnetic field lines crossing the orange cylinders are considered. The apex of each magnetic closed line is denoted by the rhomboids as in panel (a), and edged rhomboids represent the minima of the apexes inside the cylinder. Panel (c): example of the “topological” path (the orange line connecting the orange dots) calculated in a 2D example from the initial position e0. The gray lines indicate closed field lines in a pseudostreamer topology (and helmet streamer to the left) and the blue lines are open field lines.

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