422 citations · 1.9k across the 43 of their papers we have counts for
35 papers · 1 filter
CoSEE-Cat: A Comprehensive Solar Energetic Electron event Catalogue obtained from combined in situ and remote-sensing observations from Solar Orbiter -- Catalogue description and first statistical results
A. Warmuth, F. Schuller, R. Gómez-Herrero +39
(abridged) The acceleration of particles at the Sun and their propagation through interplanetary space are key topics in heliophysics. Specifically, solar energetic electrons (SEEs…
Bursty acceleration and 3D trajectories of electrons in a solar flare
Shilpi Bhunia, Laura A. Hayes, Karl Ludwig Klein +3
During a solar flare, electrons are accelerated to non-thermal energies as a result of magnetic reconnection. These electrons then propagate upwards and downwards from the energy r…
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…
Empirical atmosphere model in a mini flare during magnetic reconnection
Brigitte Schmieder, Reetika Joshi, Ramesh Chandra +6
A spatio-temporal analysis of IRIS spectra of MgII, CII, and SiIV ions allows us to study the dynamics and the stratification of the flare atmosphere along the line of sight during…
Spectral Analysis of Solar Radio Type III Bursts from 20 kHz to 410 MHz
K. Sasikumar Raja, Milan Maksimovic, Eduard P. Kontar +10
We present the statistical analysis of the spectral response of solar radio type III bursts over the wide frequency range between 20 kHz and 410 MHz. For this purpose, we have used…
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…