How Transverse Waves Drive Turbulence in the Solar Corona
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DOI: 10.3390/sym14020384
Abstract: Oscillatory power is pervasive throughout the solar corona, and magnetohydrodynamic (MHD) waves may carry a significant energy flux throughout the Sun’s atmosphere. As a result, over much of the past century, these waves have attracted… read more here.
Keywords: solar corona; waves drive; energy; transverse waves ... See more keywords