Abstract
Prominent structures and fluctuations in the solar wind appear to be closely associated with coronal magnetic structures and turbulence. Coronal hole related high-speed flows act as wave guides conducting Alfvénic fluctuations of solar origin into interplanetary space. Medium-sized plasma flow tubes seem to originate from coronal fine-structures presumed to be identical with the plumes seen in corona-graph pictures.
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Marsch, E. (1991). Signatures of Coronal Structures and Turbulence in the Solar Wind. In: Ulmschneider, P., Priest, E.R., Rosner, R. (eds) Mechanisms of Chromospheric and Coronal Heating. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-87455-0_35
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DOI: https://doi.org/10.1007/978-3-642-87455-0_35
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