activity
20072026
most citedNonlinear Instability of kink oscillations due to shear motions

183 citations · 2.8k across the 67 of their papers we have counts for

collaborators

66 papers

astro-ph.SR2026

Reevaluating thermal instability in a uniform plasma: an extended analysis of instability domains

Varsha Felsy, Ramon Oliver, Jaume Terradas +3

Thermal instability plays a crucial role in the dynamics of astrophysical plasmas. Building upon the foundational work of G. B. Field (1965) and the subsequent analysis by T. Water…

astro-ph.SR2023

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…

astro-ph.SR2023★ 7 cited

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…

astro-ph.SR2022★ 4 cited

Three-dimensional solar active region magnetohydrostatic models and their stability using Euler potentials

Jaume Terradas, Thomas Neukirch

Active regions (ARs) are typical magnetic structures found in the solar atmosphere. We calculate several magnetohydrostatic (MHS) equilibrium models that include the effect of a fi…

astro-ph.SR2022★ 9 cited

Extension and validation of the pendulum model for longitudinal solar prominence oscillations

M. Luna, J. Terradas, J. Karpen +1

Longitudinal oscillations in prominences are common phenomena on the Sun. These oscillations can be used to infer the geometry and intensity of the filament magnetic field. Previou…

astro-ph.SR2022★ 6 cited

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…