Spatial damping of MHD waves in solar prominences: Effect of background flow
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DOI: 10.1016/j.asr.2021.05.009
Abstract: Abstract The extensive arch-shaped features, solar prominences, are observed subtending high into the solar corona. Considering the prominences to be unbound, homogeneous and isothermal, invoking the background flow, in presence of the Newtonian radiation and… read more here.
Keywords: background flow; effect background; spatial damping; solar prominences ... See more keywords