Element and Isotopic Fractionation in Closed Magnetic Structures

Computer Science

Scientific paper

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Solar Wind, Solar Wind Composition, Fip Fractionation, 3He/4He Fractionation, Solar Magnetic Field

Scientific paper

Recent papers have suggested that the slow solar wind is a super-position of material which is released by reconnection from large coronal loops. This reconnection process is driven by large-scale motions of solar magnetic flux driven by the non-radial expansion of the solar wind from the differentially rotating photosphere into more rigidly rotating coronal holes.

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