181 citations · 2.6k across the 66 of their papers we have counts for
66 papers
On the origins of coronal Alfvénic waves
R. J. Morton, R. Soler
Alfvénic waves are considered a key contributor to the energy flux that powers the Sun's corona, with theoretical models demonstrating their potential to explain coronal EUV and X-…
The energy content of Alfven waves in the stratified solar atmosphere
Roberto Soler
Alfven waves propagating in a vertically stratified plasma, such as those travelling from the solar photosphere to the corona, are partially reflected due to the gradient in the Al…
The role of initial density profiles in simulations of coronal wave - coronal hole interaction
I. Piantschitsch, J. Terradas, E. Soubrie +4
Interactions between global coronal waves (CWs) and coronal holes (CHs) reveal many interesting features of reflected waves and coronal hole boundaries (CHB) but have fairly been s…
Self-consistent equilibrium models of prominence thin threads heated by Alfvén waves propagating from the photosphere
Llorenç Melis, Roberto Soler, Jaume Terradas
The fine structure of solar prominences is made by thin threads that outline the magnetic field lines. Observations show that transverse waves of Alfvénic nature are ubiquitous in…
Quasimodes in the cusp continuum in nonuniform magnetic flux tubes
Michaël Geeraerts, Pieter Vanmechelen, Tom Van Doorsselaere +1
The study of MHD waves is important both for understanding heating in the solar atmosphere and for solar atmospheric seismology. The analytical investigation of wave mode propertie…
Construction of coronal hole and active region magnetohydrostatic solutions in two dimensions: Force and energy balance
J. Terradas, R. Soler, R. Oliver +7
Coronal holes and active regions are typical magnetic structures found in the solar atmosphere. We propose several magnetohydrostatic equilibrium solutions that are representative…