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Magnetic Field Geometry and Composition Variation in Slow Solar Winds: The Case of Sulfur

  • Authors: Natsuha Kuroda, and J. Martin Laming

2020 The Astrophysical Journal 895 36.

  • Provider: AAS Journals

Caption: Figure 3.

Field lines identified at the footpoint locations (orange crosses on the magnetograms) of the sulfur-enhanced slow wind (a) and of the regular slow wind (b), marked by the red and blue vertical lines in Figure 1, respectively, with corresponding EIT 195 Å images. The white, magenta, and green field lines indicate the closed, negative open, and positive open-field lines, respectively. The average magnetic field profiles of open-field lines (only negative/magenta for (a)) were used for the modeling in Section 3.

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