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20242026
most citedMagnetic Field Geometry and Anisotropic Scattering Effects on Solar Radio Burst Observations

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

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12 papers · 1 filter

astro-ph.SR2026

Energy Transport and Heating by Non-Thermal Electrons in a Turbulent Solar Flare Environment

A. Gordon Emslie, Eduard P. Kontar

The impulsive phase of a solar flare is known to generate strong turbulence and to transfer magnetic energy into accelerated electrons. Recognizing the importance of angular diffus…

astro-ph.SR2026

Constraining turbulent solar flare acceleration regions by connecting kinetic modeling and X-ray observations

Morgan Stores, Natasha Jeffrey, Ewan Dickson +2

Spatially-resolved X-ray observations are the key to understanding electron acceleration in solar flares. Currently, the underlying processes that efficiently energize solar flare…

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

Signatures of Large-Scale Magnetic Field Disturbances and Switchbacks in Interplanetary Type III Radio Bursts

Daniel L. Clarkson, Eduard P. Kontar

Type III solar radio bursts are driven by non-thermal electron beams travelling along heliospheric magnetic fields, with the radio emission frequency drift-rate determined by the b…

astro-ph.SR2025

Energy-Containing Electrons in Solar Flares: Improving Hard X-Ray and EUV Diagnostics

Yingjie Luo, Eduard P. Kontar, Debesh Bhattacharjee

Solar flares effectively accelerate particles to non-thermal energies. These accelerated electrons are responsible for energy transport and subsequent emissions in HXR, radio, and…

astro-ph.SR2025

Ion-scale Turbulence and Energy Cascade Rate in the Solar Corona and Inner Heliosphere

Eduard P. Kontar, A. Gordon Emslie, Daniel L. Clarkson +1

Plasma turbulence cascading from MHD to kinetic scales in the heliospheric plasma is believed to play a key role in coronal heating and fast solar wind acceleration, but the proper…