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

5 citations · 7 across the 12 of their papers we have counts for

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11 papers · 1 filter

astro-ph.SR2026

Mapping Oscillatory Flows in a Giant Chromospheric Spiral

Yash. B. Saneshwar, Eamon Scullion, Gert J. J. Botha

The solar chromosphere is permeated by complex magnetic fields that guide plasma flows and energy into the corona. This work presents a detailed analysis of a unique, high-resoluti…

astro-ph.SR2026

Probing the Solar Corona and the Solar Wind Using Angular Broadening Observations with the SKA

Peijin Zhang, John Morgan, Divya Oberoi +9

Angular broadening observations of compact radio sources provide a powerful method for probing the solar corona and solar wind. Such observations enable studies of the phase struct…

astro-ph.SR2026

First Detailed MeerKAT Imaging Spectroscopy of a Solar Flare

Yingjie Luo, Eduard P. Kontar, Roelf Du Toit Strauss +5

Radio observations provide powerful diagnostics of energy release, particle acceleration, and transport processes in solar flares. However, despite recent progress in radio interfe…

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…