activity
20032026
most citedObservational Tests of Damping by Resonant Absorption in Coronal Loop Oscillations

190 citations · 2.9k across the 86 of their papers we have counts for

collaborators

88 papers

astro-ph.SR2026

Streamer slab eigenmode analysis with the Legolas code

Jordi De Jonghe, Daria Sorokina, Tom Van Doorsselaere

Context. Helmet streamers are large ray-like structures extending from the solar corona that thin further away from the solar surface, forming an extended current sheet. These stru…

astro-ph.SR2026

A Self-consistent Model for the Generation of Coronal Condensations: The Effects of Turbulent Wave Dissipation

M. McMurdo, V. Jercic, T. Van Doorsselaere +1

Prominences and coronal rain are two manifestations of coronal condensations whose formation mechanisms remain only partially understood. While previous studies have explored how l…

astro-ph.SR2026

Fast and periodic propagating disturbances along coronal loops detected with EUI on board Solar Orbiter

A. Dolliou, S. Mandal, K. Barczynski +9

Recent high-resolution observations from the Solar Orbiter mission can help detect the indirect signatures of heating at the smallest scales. In this work we measure the properties…

physics.plasm-ph2026

Rankine-Hugoniot conditions in Q-variables: a wave-aligned formulation of MHD discontinuities

Anna Krupka, Tijs Van Hoof, Tom Van Doorsselaere

The recently developed Q-variable formalism generalises the Elsässer representation by providing a wave-aligned representation applicable to a broad class of magnetohydrodynamic di…

astro-ph.SR2026

Imaging magnetically driven astrospheres: a forward modelling approach

Ziqi Wu, Tom Van Doorsselaere, Jiansen He +5

An astrosphere is a vast, tailed bubble-like volume around a star, formed through the interaction between the stellar magnetic field, the stellar wind, and the interstellar medium…

physics.plasm-ph2026

Numerical simulations of waves and turbulence in coronal loops: observables and spectra

Fabio Feraco, Francesco Pucci, Claudio Meringolo +11

We investigate numerically the time evolution of velocity and magnetic field fluctuations in a coronal loop, focusing on the dynamics due to both phase mixing and turbulent cascade…