Coronal transverse magnetohydrodynamic waves in a solar prominence
Abstract
Solar prominences are cool 104 Kelvin plasma clouds supported in the surrounding 106 Kelvin coronal plasma by as-yet undetermined mechanisms. Observations from Hinode show fine-scale threadlike structures oscillating in the plane of the sky with periods of several minutes. We suggest these transverse magnetohydrodynamic waves may represent Alfv\'en waves propagating on coronal magnetic field lines and these may play a role in heating the corona.
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