activity
20232025
most citedAn Anisotropic Density Turbulence Model from the Sun to 1 au Derived From Radio Observations

35 citations · 50 across the 5 of their papers we have counts for

collaborators

5 papers

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.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…

astro-ph.SR2023★ 35 cited

An Anisotropic Density Turbulence Model from the Sun to 1 au Derived From Radio Observations

Eduard P. Kontar, A. Gordon Emslie, Daniel L. Clarkson +5

Solar radio bursts are strongly affected by radio-wave scattering on density inhomogeneities, changing their observed time characteristics, sizes, and positions. The same turbulenc…

astro-ph.SR2023★ 15 cited

Source positions of an interplanetary type III radio burst and anisotropic radio-wave scattering

Xingyao Chen, Eduard P. Kontar, Nicolina Chrysaphi +7

Interplanetary solar radio type III bursts provide the means for remotely studying and tracking energetic electrons propagating in the interplanetary medium. Due to the lack of dir…