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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

A Multispacecraft Analysis and Modeling of Type III Radio Burst Exciter Deceleration in Inhomogeneous Heliospheric Plasma

Francesco Azzollini, Eduard P. Kontar

Electron beams accelerated in solar flares and escaping from the Sun along open magnetic field lines can trigger intense radio emissions known as type III solar radio bursts. Utili…

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…

astro-ph.SR2025

Total Power and Low-energy Cut-off Time Evolution of Solar Flare Accelerated Electrons Using X-Ray Observations and Warm-Target Model

Debesh Bhattacharjee, Eduard P. Kontar, Yingjie Luo

A primary characteristic of solar flares is the efficient acceleration of electrons to nonthermal deka-keV energies. While hard X-Ray (HXR) observation of bremsstrahlung emission s…

astro-ph.SR2025

Tracing the Heliospheric Magnetic Field via Anisotropic Radio-Wave Scattering

Daniel L. Clarkson, Eduard P. Kontar, Nicolina Chrysaphi +4

Astrophysical radio sources are embedded in turbulent magnetised environments. In the 1 MHz sky, solar radio bursts are the brightest sources, produced by electrons travelling alon…