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astro-ph.SR2024
Advection-nonlinear-diffusion model of flare accelerated electron transport in Type III solar radio bursts
Eduard P. Kontar, Francesco Azzollini, Olena Lyubchyk
Electrons accelerated by solar flares and observed as type III solar radio bursts are not only a crucial diagnostic tool for understanding electron transport in the inner heliosphe…
astro-ph.SR2024
Plasma motions and compressive wave energetics in the solar corona and solar wind from radio wave scattering observations
Francesco Azzollini, A. Gordon Emslie, Daniel L. Clarkson +2
Radio signals propagating via the solar corona and solar wind are significantly affected by compressive waves, impacting properties of solar bursts as well as sources viewed throug…