205 citations · 306 across the 9 of their papers we have counts for
9 papers
Bayesian evidence for two slow-wave damping models in hot coronal loops
I. Arregui, D. Y. Kolotkov, V. M. Nakariakov
We compute the evidence in favour of two models, one based on field-aligned thermal conduction alone and another that includes thermal misbalance as well, in explaining the damping…
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…
Resonant absorption: transformation of compressive motions into vortical motions
M. Goossens, I. Arregui, R. Soler +1
This paper investigates the changes in spatial properties when magnetohydrodynamic (MHD) waves undergo resonant damping in the Alfvén continuum. The analysis is carried out for a 1…
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…
Analytic approximate seismology of propagating MHD waves in the solar corona
M. Goossens, R. Soler, I. Arregui +1
Observations show that propagating magnetohydrodynamic (MHD) waves are ubiquitous in the solar atmosphere. The technique of MHD seismology uses the wave observations combined with…
Prominence seismology
I. Arregui, J. L. Ballester, R. Oliver +2
Given the difficulty in directly determining prominence physical parameters from observations, prominence seismology stands as an alternative method to probe the nature of these st…
Bayesian Magnetohydrodynamic Seismology of Coronal Loops
Inigo Arregui, Andres Asensio Ramos
We perform a Bayesian parameter inference in the context of resonantly damped transverse coronal loop oscillations. The forward problem is solved in terms of parametric results for…
Three-Dimensional Propagation of Magnetohydrodynamic Waves in Solar Coronal Arcades
S. Rial, I. Arregui, J. Terradas +2
We numerically investigate the excitation and temporal evolution of oscillations in a two-dimensional coronal arcade by including the three-dimensional propagation of perturbations…
On the nature of kink MHD waves in magnetic flux tubes
M. Goossens, J. Terradas, J. Andries +2
Magnetohydrodynamic (MHD) waves are often reported in the solar atmosphere and usually classified as slow, fast, or Alfvén. The possibility that these waves have mixed properties i…