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- W2487059347 abstract "Abstract The solar corona – one of the most spectacular celestial shows and yet one of the most challenging puzzles – exhibits a spectrum of structures related to both the quiet Sun and active regions. In spite of dramatic differences in appearance and physical processes, all these structures share a common origin: they are all related to the solar magnetic field. The origin of the field is beneath the turbulent convection zone, where the magnetic field is not a master but a slave, and one can wonder how much the coronal magnetic field “remembers” its dynamo origin. Surprisingly, it does. We will describe several observational phenomena that indicate a close relationship between coronal and sub-photospheric processes." @default.
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- W2487059347 date "2000-01-01" @default.
- W2487059347 modified "2023-09-25" @default.
- W2487059347 title "Coronal Structures as Tracers of Sub-Surface Processes" @default.
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- W2487059347 doi "https://doi.org/10.1017/s0252921100064460" @default.
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