Spatial damping of MHD waves in solar prominences: Effect of background flow
Sign Up to like & getrecommendations! Published in 2021 at "Advances in Space Research"
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
Modeling of the Fine Filament Structure of Quiescent Solar Prominences
Sign Up to like & getrecommendations! Published in 2017 at "Geomagnetism and Aeronomy"
DOI: 10.1134/s0016793217080138
Abstract: Several new models of solar prominences with helical geometry of the magnetic field were suggested; the possibility of the construction of a filament model with a fine filament structure was shown. For the first time,… read more here.
Keywords: fine filament; filament structure; structure; filament ... See more keywords