Abstract
The Sun is our nearest star. It is important for astronomy because many phenomena which can only be studied indirectly in other stars can be directly observed in the Sun (e.g. stellar rotation, starspots, the structure of the stellar surface). Our present picture of the Sun is based both on observations and on theoretical calculations. Some observations of the Sun disagree with the theoretical solar models. The details of the models will have to be changed, but the general picture should remain valid.
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References
Noyes, R. W. (1982): The Sun, Our Star (Harvard University Press, Cambridge, MA)
Priest, E. R. (1982): Solar Magnetohydrodynamics (Reidel, Dordrecht)
Stix, M. (1989): The Sun — An Introduction (Springer, Berlin, Heidelberg)
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© 1994 Springer-Verlag Berlin Heidelberg
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Karttunen, H., Kröger, P., Oja, H., Poutanen, M., Donner, K.J. (1994). The Sun. In: Karttunen, H., Kröger, P., Oja, H., Poutanen, M., Donner, K.J. (eds) Fundamental Astronomy. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-11794-1_13
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DOI: https://doi.org/10.1007/978-3-662-11794-1_13
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-57203-9
Online ISBN: 978-3-662-11794-1
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