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Electromagnetic wave lensing, a common physical phenomenon recognized in visible light for centuries, finds extensive applications in manipulating light in optical systems such as telescopes and cameras. Magnetohydrodynamic wave is a common perturbation phenomenon in the corona. By using high spatio-temporal resolution observations from the Solar Dynamics Observatory, here, we report the observation of a magnetohydrodynamic wave lensing in the ...

Publications

From eruption to post-flare rain: A 2.5D MHD model KU Leuven

Mass Cycle and Dynamics of a Virtual Quiescent Prominence KU Leuven

BxC Toolkit: Generating Tailored Turbulent 3D Magnetic Fields KU Leuven

A spectroscopic investigation of thermal instability for cylindrical equilibria with background flow KU Leuven

Radiative loss and ion-neutral collisional effects in astrophysical plasmas KU Leuven

Frozen-field Modeling of Coronal Condensations with MPI-AMRVAC. I. Demonstration in Two-dimensional Models KU Leuven

The Lorentz Force at Work: Multiphase Magnetohydrodynamics throughout a Flare Lifespan KU Leuven

Parametric Survey of Nonaxisymmetric Accretion Disk Instabilities: Magnetorotational Instability to Super-Alfvénic Rotational Instability KU Leuven

Exploring self-consistent 2.5D flare simulations with MPI-AMRVAC KU Leuven

Resolved magnetohydrodynamic wave lensing in the solar corona KU Leuven