181 citations · 2.6k across the 66 of their papers we have counts for
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Solar prominences embedded in flux ropes: morphological features and dynamics from 3D MHD simulations
J. Terradas, R. Soler, M. Luna +3
The temporal evolution of a solar prominence inserted in a three-dimensional magnetic flux rope is investigated numerically. Using the model of Titov Demoulin (1999) under the regi…
Dynamics of coronal rain and descending plasma blobs in solar prominences: II. partially ionized case
R. Oliver, R. Soler, J. Terradas +1
Coronal rain clumps and prominence knots are dense condensations with chromospheric to transition region temperatures that fall down in the much hotter corona. Their typical speeds…
Model comparison for the density structure across solar coronal waveguides
I. Arregui, R. Soler, A. Asensio Ramos
The spatial variation of physical quantities, such as the mass density, across solar atmospheric waveguides governs the timescales and spatial scales for wave damping and energy di…
Damped transverse oscillations of interacting coronal loops
Roberto Soler, Manuel Luna
Damped transverse oscillations of magnetic loops are routinely observed in the solar corona. This phenomenon is interpreted as standing kink magnetohydrodynamic waves, which are da…
On the spatial scales of wave heating in the solar chromosphere
Roberto Soler, Marc Carbonell, Jose Luis Ballester
Dissipation of magnetohydrodynamic (MHD) wave energy has been proposed as a viable heating mechanism in the solar chromospheric plasma. Here, we use a simplified one-dimensional mo…
Model comparison for the density structure along solar prominence threads
I. Arregui, R. Soler
Quiescent solar prominence fine structures are typically modelled as density enhancements, called threads, which occupy a fraction of a longer magnetic flux tube. The profile of th…