Figure 5 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 5.

Fractionations with respect to O for Mg, Fe, Si, S, N, Ne, and He, plotted for epochs 0, 2, 4, 6 (black data points). Model fractionations give different proportions of plasma fractionated in open and closed fields. Open fields favors high S/O and high He/O.

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