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• W1865960812 abstract "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." @default.
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• W1865960812 date "1998-01-01" @default.
• W1865960812 modified "2023-09-28" @default.
• W1865960812 title "Element and Isotopic Fractionation in Closed Magnetic Structures" @default.
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• W1865960812 doi "https://doi.org/10.1007/978-94-011-4820-7_36" @default.
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