Abstract
In this chapter we will explain the basic MHD equations which are needed to understand solar active phenomena such as spots, prominences, flares etc. The solar dynamo is needed to maintain the solar activity cycle1.
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© 2007 Springer
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HANSLMEIER, A. (2007). MHD and the Solar Dynamo. In: THE SUN AND SPACE WEATHER. ASTROPHYSICS AND SPACE SCIENCE LIBRARY, vol 347. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5604-8_4
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DOI: https://doi.org/10.1007/978-1-4020-5604-8_4
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-5603-1
Online ISBN: 978-1-4020-5604-8
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