49 citations · 136 across the 6 of their papers we have counts for
6 papers
Can we rely on EUV emission to identify coronal waveguides?
P. Kohutova, P. Antolin, M. Szydlarski +1
Traditional models of coronal oscillations rely on modelling the coronal structures that support them as compact cylindrical waveguides. Recently, an alternative model of the struc…
Damping of coronal oscillations in self-consistent 3D radiative MHD simulations of the solar atmosphere
P. Kohutova, P. Antolin, M. Szydlarski +1
Oscillations are abundant in the solar corona. Coronal loop oscillations are typically studied using highly idealised models of magnetic flux tubes. In order to improve our underst…
High-resolution observations of the solar photosphere, chromosphere and transition region. A database of coordinated IRIS and SST observations
L. H. M. Rouppe van der Voort, B. De Pontieu, M. Carlsson +30
NASA's Interface Region Imaging Spectrograph (IRIS) provides high resolution observations of the solar atmosphere through UV spectroscopy and imaging. Since the launch of IRIS in J…
First direct observation of a torsional Alfvén oscillation at coronal heights
P. Kohutova, E. Verwichte, C. Froment
Torsional Alfvén waves are promising candidates for transport of energy across different layers of the solar atmosphere and have been theoretically predicted for decades. Previous…
Multi-scale observations of thermal non-equilibrium cycles in coronal loops
C. Froment, P. Antolin, V. M. J. Henriques +2
Thermal non-equilibrium (TNE) is a phenomenon that can occur in solar coronal loops when the heating is quasi-constant and highly-stratified. Under such heating conditions, coronal…
Formation of coronal rain triggered by impulsive heating associated with magnetic reconnection
P. Kohutova, E. Verwichte, C. Froment
Coronal rain consists of cool plasma condensations formed in coronal loops as a result of thermal instability. The standard models of coronal rain formation assume that the heating…