MHD turbulence and heating of the open field-line solar corona

This paper discusses the possibility that heating of the solar corona in open field-line regions emanating from coronal holes is due to a nonlinear cascade, driven by low-frequency or quasi-static magnetohydrodynamic fluctuations. Reflection from coronal inhomogeneities plays an important role in su...

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Bibliographic Details
Published in:Nonlinear Processes in Geophysics
Main Authors: Matthaeus, William H., Mullan, D. J., Dmitruk, Pablo, Milano, L. J., Oughton, Sean
Format: Article in Journal/Newspaper
Language:English
Published: European Geoscience Union 2003
Subjects:
Online Access:https://hdl.handle.net/10289/8627
https://doi.org/10.5194/npg-10-93-2003