152 citations · 996 across the 39 of their papers we have counts for
39 papers
Coronal electron density: Insights from radio and in situ observations, and EUHFORIA modeling
Ketaki Deshpande, Jasmina Magdalenic, Immanuel Christopher Jebaraj +4
The distribution of the coronal electron density at different distances from the Sun strongly influences the physical processes in the solar corona and is therefore a very importan…
Clustering Wind data at 1 AU to contextualize magnetic reconnection in the solar wind
Francesco Carella, Giovanni Lapenta, Alessandro Bemporad +4
Context. Magnetic reconnection events are frequently observed in the solar wind. Understanding the patterns and structures within the solar wind is crucial to put observed magnetic…
On the source sizes of type II radio bursts with LOFAR
A. Kumari, D. E. Morosan, V. Mugundhan +5
Solar radio bursts can provide important insights into the underlying physical mechanisms that drive the small and large-scale eruptions on the Sun. Since metric radio observations…
Calibrating the WSA model in EUHFORIA based on PSP observations
Evangelia Samara, Charles N. Arge, Rui F. Pinto +5
We employ Parker Solar Probe (PSP) observations during the latest solar minimum period (years 2018 -2021) to calibrate the version of the Wang-Sheeley-Arge (WSA) coronal model used…
Electron Cyclotron Maser Emission and the Brightest Solar Radio Bursts
Stephen M. White, Masumi Shimojo, Kazumasa Iwai +5
This paper investigates the incidence of coherent emission in solar radio bursts, using a revised catalog of 3800 solar radio bursts observed by the Nobeyama Radio Polarimeters fro…
Fundamental-harmonic pairs of interplanetary type III radio bursts
Immanuel Christopher Jebaraj, Vladimir Krasnoselskikh, Marc Pulupa +2
Type III radio bursts are not only the most intense but also the most frequently observed solar radio bursts. However, a number of their defining features remain poorly understood.…