most citedThe periodicity of three-dimensional oscillatory reconnection

1 citations · 2 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR20261 cited

Fast Magnetoacoustic Wave Behavior within Gravitationally Stratified, Magnetically Inhomogeneous Media

Ryan T. Smith, James A. McLaughlin, Gert J. J. Botha

The nature of MHD waves within inhomogeneous media is fundamental to understanding and interpreting wave behavior in the solar atmosphere. We investigate fast magnetoacoustic wave…

astro-ph.SR2026

Wave generation via oscillatory reconnection at a three-dimensional magnetic null point

Luiz A. C. A. Schiavo, Gert J. J. Botha, James A. McLaughlin

This work conducts a three-dimensional (3D), nonlinear magnetohydrodynamic (MHD) simulation to investigate wave generating, time-dependent reconnection around a magnetic null point…

astro-ph.SR2025

Time-dependent Turbulent Electron Acceleration and Transport in Solar Flares

Luiz A. C. A. Schiavo, Natasha L. S. Jeffrey, Gert J. J. Botha +1

Solar flares are explosive releases of magnetic energy stored in the solar corona, driven by magnetic reconnection. These events accelerate electrons, generating hard X-ray emissio…

astro-ph.SR20251 cited

The periodicity of three-dimensional oscillatory reconnection

Luiz A. C. A. Schiavo, Gert J. J. Botha, James A. McLaughlin

Oscillatory reconnection is a dynamic, magnetic relaxation mechanism in which a perturbed null point reverts back to equilibrium via time-dependent reconnection. In this paper, we…

astro-ph.SR2025

Solar Vortices as Conduits for Magnetoacoustic Waves: Multi-Layer Coupling and Their Role in Atmospheric Heating

Suzana S. A. Silva, Ioannis Dakanalis, Luiz A. C. A. Schiavo +10

The Sun's atmosphere hosts swirling plasma structures, known as solar vortices, which have long been thought to channel wave energy into higher layers. Until now, no direct observa…

astro-ph.SR2025

The coronal power spectrum from MHD mode conversion above sunspots

Hemanthi Miriyala, Richard J. Morton, Elena Khomenko +2

Sunspots are intense regions of magnetic flux that are rooted deep below the photosphere. It is well established that sunspots host magnetohydrodynamic waves, with numerous observa…