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

35 citations · 69 across the 7 of their papers we have counts for

collaborators

7 papers

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.SR2024

First determination of the angular dependence of rise and decay times of solar radio bursts using multi-spacecraft observations

Nicolina Chrysaphi, Milan Maksimovic, Eduard P. Kontar +3

Radio photons interact with anisotropic density fluctuations in the heliosphere, which can alter their trajectory and influence properties deduced from observations. This is partic…

physics.space-ph2024

Acceleration and Release of Solar Energetic Particles Associated with a Coronal Shock on 2021 September 28 Observed by Four Spacecraft

Bin Zhuang, Noé Lugaz, David Lario +5

Extreme ultraviolet (EUV) waves are thought to be the propagating footprint of the shock on the solar surface. One of the key questions in SEP research is the timing of the SEP rel…

astro-ph.SR202335 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.SR202318 cited

Total Electron Temperature Derived from Quasi-Thermal Noise Spectroscopy In the Pristine Solar Wind: Parker Solar Probe Observations

M. Liu, K. Issautier, M. Moncuquet +11

The Quasi-thermal noise (QTN) technique is a reliable tool to yield accurate measurements of the electron parameters in the solar wind. We apply this method on Parker Solar Probe (…

astro-ph.SR202311 cited

Solar Radio Spikes and Type IIIb Striae Manifestations of Sub-second Electron Acceleration Triggered by a Coronal Mass Ejection

Daniel L. Clarkson, Eduard P. Kontar, Nicole Vilmer +3

Understanding electron acceleration associated with magnetic energy release at sub-second scales presents a major challenges in solar physics. Solar radio spikes observed as sub-se…