activity
20242026
collaborators

18 papers

astro-ph.IM2026

Astrophysics on GPUs: introducing AGILE 1.0

Oliver Porth, Adrian Kelly, Olaf Willocx +10

We present AGILE, a GPU-enabled adaptive mesh refinement (AMR) framework for the solution of (near-) conservation laws which occur in astro- and solar-physical applications. AGILE…

astro-ph.SR2026

Once more: Leaky MHD waves in coronal magnetic flux tubes

Hans Goedbloed, Rony Keppens

By a detailed comparison of leaky magnetohydrodynamic waves in coronal magnetic flux tubes with leaky electromagnetic waves in dielectric media it is shown that the latter kind may…

physics.space-ph2026

High-energy Particle Transport in Three-dimensional Anisotropic Turbulent Magnetic Fields

Daniela Maci, Rony Keppens, Fabio Bacchini

The understanding and modeling of high-energy particles transport in turbulent magnetic fields is an important open question in space- and astrophysics. The multiscale, nonlinear n…

astro-ph.SR2026

Thermal instability in coronal loops: linking eigenvalue spectra to time-dependent evolution

Adrian Kelly, Rony Keppens, Jordi De Jonghe

Cool, dense condensations such as coronal rain and prominences suggest that coronal plasma can undergo runaway radiative cooling. Connecting this behaviour to linear thermal modes…

astro-ph.SR2026

On the dynamics, thermodynamics and fine structure of virtual erupting filaments

Dion Donné, Yuhao Zhou, Hebe Cremades +1

It is not fully understood why some solar filaments erupt while others do not. Those that do typically undergo a slow rise followed by an acceleration phase, though this transition…

astro-ph.SR2026

Nonthermal electron acceleration in turbulent post-flare coronal loops

Clarissa Mora, Fabio Bacchini, Rony Keppens

The generation of nonthermal electrons during solar flares plays a critical role in energy transport from the corona to the chromosphere, producing regions of observed intense X-ra…