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- W2010461605 abstract "Observations nowadays reveal more and more details about the small-scale structure of the penumbra and umbra. Recent measurements of the motions in the penumbra indicate that (i) the Evershed flow is confined to a thin photospheric layer and (ii) the material rises from and sinks to subphotospheric layers within the penumbra. This flow pattern solves the question of the mass budget of the Evershed flow in a natural way. The nature of umbral dots and their role for the spot's energy budget remains unclear, since they are obviously unresolved even in the best existing measurements." @default.
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- W2010461605 date "2003-06-01" @default.
- W2010461605 modified "2023-10-18" @default.
- W2010461605 title "Material flow in sunspots" @default.
- W2010461605 doi "https://doi.org/10.1002/asna.200310133" @default.
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