activity
19992025
most citedGlobal Energetics of Thirty-Eight Large Solar Eruptive Events

491 citations · 1.8k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.SR2025★ 2 cited

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★ 9 cited

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…

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★ 9 cited

The efficiency of electron acceleration during the impulsive phase of a solar flare

Eduard P. Kontar, A. Gordon Emslie, Galina G. Motorina +1

Solar flares are known to be prolific electron accelerators, yet identifying the mechanism(s) for such efficient electron acceleration in solar flare (and similar astrophysical set…

astro-ph.IM2023★ 11 cited

Robust construction of differential emission measure profiles using a regularized maximum likelihood method

Paolo Massa, A. Gordon Emslie, Iain G. Hannah +1

Extreme-ultraviolet (EUV) observations provide considerable insight into evolving physical conditions in the active solar atmosphere. For a prescribed density and temperature struc…