activity
20182021
most citedFirst Observation of a Type II Solar Radio Burst Transitioning Between a Stationary and Drifting State

32 citations · 92 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202112 cited

First Frequency-Time-Resolved Imaging Spectroscopy Observations of Solar Radio Spikes

Daniel L. Clarkson, Eduard P. Kontar, Mykola Gordovskyy +2

Solar radio spikes are short duration and narrow bandwidth fine structures in dynamic spectra observed from GHz to tens of MHz range. Their very short duration and narrow frequency…

astro-ph.SR2021

Fine structures of solar radio bursts: origins and radio-wave propagation effects

Nicolina Chrysaphi

The abstract is available at: http://dx.doi.org/10.5525/gla.thesis.82010

astro-ph.SR202024 cited

Sub-second time evolution of Type III solar radio burst sources at fundamental and harmonic frequencies

Xingyao Chen, Eduard P. Kontar, Nicolina Chrysaphi +4

Recent developments in astronomical radio telescopes opened new opportunities in imaging and spectroscopy of solar radio bursts at sub-second timescales. Imaging in narrow frequenc…

astro-ph.SR202024 cited

Radio Echo in the Turbulent Corona and Simulations of Solar Drift-Pair Radio Bursts

Alexey A. Kuznetsov, Nicolina Chrysaphi, Eduard P. Kontar +1

Drift-pair bursts are an unusual type of solar low-frequency radio emission, which appear in the dynamic spectra as two parallel drifting bright stripes separated in time. Recent i…

astro-ph.SR202032 cited

First Observation of a Type II Solar Radio Burst Transitioning Between a Stationary and Drifting State

Nicolina Chrysaphi, Hamish A. S. Reid, Eduard P. Kontar

Standing shocks are believed to be responsible for stationary Type II solar radio bursts, whereas drifting Type II bursts are excited by moving shocks often related to coronal mass…

astro-ph.SR2019

Anisotropic Radio-Wave Scattering and the Interpretation of Solar Radio Emission Observations

Eduard P. Kontar, Xingyao Chen, Nicolina Chrysaphi +6

The observed properties (i.e., source size, source position, time duration, decay time) of solar radio emission produced through plasma processes near the local plasma frequency, a…