activity
20192026
most citedCoronal Hole Detection and Open Magnetic Flux

51 citations · 411 across the 34 of their papers we have counts for

collaborators
Showing 2025Show all

8 papers · 1 filter

astro-ph.SR2025

Coronal flux tube illuminated by strong shock spot: New Year's Eve solar eruption of 2023-Dec-31

Illya Plotnikov, Alexis P. Rouillard, Athanasios Kouloumvakos +1

Powerful solar eruptions are known to produce fast and wide shock waves in the solar corona and inner heliosphere. The relationship between the coronal shock waves, solar energetic…

astro-ph.SR2025★ 2 cited

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…

astro-ph.SR2025★ 1 cited

Modelling gyrosynchrotron emission from coronal energetic electrons in a CME flux rope

Edin Husidic, Nicolas Wijsen, Immanuel Christopher Jebaraj +4

Solar flares and coronal mass ejections (CMEs) can accelerate electrons, causing bursts such as type IV emissions in the solar radio continuum. Although radio spectroscopy is a pow…

astro-ph.SR2025

Plasma instability in the front of ejected energetic electrons and Type III solar radiobursts

Vladimir Krasnoselskikh, Immanuel Christopher Jebaraj, Tom Robert Franck Cooper +7

Type III radio bursts are a signature of the flux of near-relativistic electrons ejected during solar flares. These bursts are frequently observed by spacecraft such as the Parker…

physics.space-ph2025★ 3 cited

Freely propagating flanks of wide coronal-mass-ejection-driven shocks: Modelling and observational insights

N. Wijsen, I. C. Jebaraj, N. Dresing +3

Widespread solar energetic particle (SEP) events remain poorly understood phenomena in space weather. These events are often linked to coronal mass ejections (CMEs) and their shock…

astro-ph.SR2025★ 6 cited

Resolving spatial and temporal shock structures using LOFAR observations of type II radio bursts

D. E. Morosan, I. C. Jebaraj, P. Zhang +6

Collisionless shocks are one of the most powerful particle accelerators in the Universe. In the heliosphere, type II solar radio bursts are signatures of electrons accelerated by c…

astro-ph.SR2025★ 11 cited

On the reason for the widespread energetic storm particle event of 13 March 2023

N. Dresing, I. C. Jebaraj, N. Wijsen +20

On 13 March 2023, when the Parker Solar Probe was situated on the far side of the Sun as seen from Earth, a large solar eruption took place creating a strong solar energetic partic…

astro-ph.SR2025★ 12 cited

Shock and SEP Modeling Study for the 5 September 2022 SEP Event

A. Kouloumvakos, N. Wijsen, I. C. Jebaraj +10

On September 5, 2022, during Parker Solar Probe's (PSP) 13th encounter, a fast shock wave and a related solar energetic particle (SEP) event were observed as the spacecraft approac…