Figure 6 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 6.

Fractionations with respect to O for Mg, Fe, Si, S, N, Ne, and He, plotted for epochs 1, 3, 5 (black data points). Model fractionations give different proportions of plasma fractionated in open and closed fields.

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