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20232026
most citedSelf-similar solutions of oscillatory reconnection: parameter study of magnetic field strength and background temperature

5 citations · 12 across the 13 of their papers we have counts for

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Showing 2025 · astro-ph.SRShow all

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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.SR2025★ 1 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

Multi-wavelength observations of substructures in solar flare ribbons

Vishal Singh, Eamon Scullion, Gert J. J. Botha +6

Solar flare ribbons are extensive brightenings in the chromosphere during flares, often showing fine scale structuring that reflects the underlying energy release. Using high caden…

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…