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- W3010438564 abstract "Abstract Surface flux transport (SFT) models have been successful in reproducing how magnetic flux at the solar photosphere evolves on large scales. SFT modelling proved to be useful in reconstructing secular irradiance variations of the Sun, and it can be potentially used in forward modelling of brightness variations of Sun-like stars. We outline our current understanding of solar and stellar SFT processes, and suggest that nesting of activity can play an important role in shaping large-scale patterns of magnetic fields and brightness variability." @default.
- W3010438564 created "2020-03-13" @default.
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- W3010438564 date "2018-08-01" @default.
- W3010438564 modified "2023-09-27" @default.
- W3010438564 title "Large-scale transport of solar and stellar magnetic flux" @default.
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- W3010438564 doi "https://doi.org/10.1017/s1743921319004587" @default.
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