Abstract
In the preceding chapters we have learned about convection and rotation, the main causes of solar magnetism. And we have learned about this magnetism itself. We shall now recognize that the Sun’s magnetic field is the main source of all the structure and variability which we find in its outermost layers: the chromosphere, the corona, and the solar wind. Moreover, we shall see that the very existence of these outer layers is most certainly due to the solar magnetic field.
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© 1989 Springer-Verlag Berlin Heidelberg
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Stix, M. (1989). Chromosphere, Corona, and Solar Wind. In: The Sun. Astronomy and Astrophysics Library. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-97129-7_9
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DOI: https://doi.org/10.1007/978-3-642-97129-7_9
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-53796-0
Online ISBN: 978-3-642-97129-7
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