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...
Published in: | Nonlinear Processes in Geophysics |
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Main Authors: | , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
European Geoscience Union
2003
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Subjects: | |
Online Access: | https://hdl.handle.net/10289/8627 https://doi.org/10.5194/npg-10-93-2003 |