Figure 4 from Magnetic Field Geometry and Composition Variation in Slow Solar Winds: The Case of Sulfur

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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 4.

Average magnetic field profiles for the open-field lines identified at the source regions of sulfur-enhanced solar winds and regular solar winds. The fields are stronger for the former because they all emanate from the region near active regions.

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