From the 2 of 22 linked papers with an AI index.
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Magnetic Field Geometry and Anisotropic Scattering Effects on Solar Radio Burst Observations
Daniel L. Clarkson, Eduard P. Kontar
The fine structures of solar radio bursts reveal complex dynamics in the corona, yet the observed characteristics of these sub-second bursts are additionally complicated by radio w…
Temporally resolved Type III solar radio bursts in the frequency range 3-13 MHz
Antonio Vecchio, Milan Maksimovic, Nicolina Chrysaphi +2
Radio observations from space allow to characterize solar radio bursts below the ionospheric cutoff, which are otherwise inaccessible, but suffer from low, insufficient temporal re…
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…