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Physics of Stellar Coronae

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Turbulence in Space Plasmas

Part of the book series: Lecture Notes in Physics ((LNP,volume 778))

For the plasma physicist, the solar corona offers an outstanding example of a space plasma, and surely one that deserves a lifetime of study. Not only can we observe the solar corona on scales of a few hundred kilometers and monitor its changes in the course of seconds to minutes but we also have a wide range of detailed diagnostics at our disposal that provide immediate access to the prevalent physical processes.

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    Güdel, M. (2009). Physics of Stellar Coronae. In: Cargill, P., Vlahos, L. (eds) Turbulence in Space Plasmas. Lecture Notes in Physics, vol 778. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-00210-6_8

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