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• W3099271491 abstract "Aims. Twisted magnetic fields are frequently seen to emerge above the visible surface of the Sun. This emergence is usually associated with the rise of buoyant magnetic flux structures. Here we ask how magnetic fields from a turbulent large-scale dynamo appear above the surface if there is no magnetic buoyancy." @default.
• W3099271491 created "2020-11-23" @default.
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• W3099271491 date "2010-11-01" @default.
• W3099271491 modified "2023-09-25" @default.
• W3099271491 title "Surface appearance of dynamo-generated large-scale fields" @default.
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• W3099271491 doi "https://doi.org/10.1051/0004-6361/201014287" @default.
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