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From the 1 of 7 linked papers with an AI index.

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20242026
most citedMeV-peaked electrons in a coronal source of a solar flare

3 citations · 3 across the 4 of their papers we have counts for

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astro-ph.SR2026

Probing the Physics of the Solar Corona with High-Resolution Observations using SKA-Mid

Mark C. M. Cheung, John S. Morgan, Rohit Sharma +3

The paper evaluates how the SKA-Mid radio telescope can be used to observe fine‑scale structures and plasma processes in the solar corona by synthesizing radio emission from radiat…

astro-ph.SR2026

Spectral evolution of mildly relativistic electrons in solar flares

Gregory D. Fleishman, Tatyana Kaltman, Sijie Yu +1

Solar flares are a powerful engine capable of accelerating ambient plasma particles to high nonthermal energies. A key characteristic of these particles is their energy spectrum. N…

astro-ph.SR2026

Modeling the Thermal Low-Frequency Radio Sun with Ray Tracing

Peijin Zhang, Bin Chen, Gregory Fleishman +4

Incoherent radio emission at meter--decimeter wavelengths provides a key diagnostic of the coronal thermal plasma, but at frequencies below \,1\,GHz coronal refraction can su…

astro-ph.SR2026

Dynamics of the coronal magnetic field in the 2022-10-02 X-class flare

Gregory D. Fleishman, Tatyana Kaltman, Sijie Yu

Solar flares are driven by release of free magnetic energy and often associated with restructurization of the magnetic field topology. Yet, observations of evolving magnetic field…

astro-ph.SR20263 cited

MeV-peaked electrons in a coronal source of a solar flare

Gregory D. Fleishman, Ivan Oparin, Gelu M. Nita +3

Analysis of γ-rays in solar flares has suggested a distinct continuum component dominating at MeV energies, which differs from the well-studied X-ray continuum produced by flare-a…