activity
20142026
most citedLOFAR tied-array imaging of Type III solar radio bursts

78 citations · 165 across the 17 of their papers we have counts for

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Showing 2025Show all

5 papers · 1 filter

astro-ph.SR2025★ 12 cited

Radio Burst from a Stellar Coronal Mass Ejection

J. R. Callingham, C. Tasse, R. Keers +15

Coronal mass ejections (CMEs) are massive expulsions of magnetised plasma from a star, and are the largest contributors to space weather in the Solar System. CMEs are theorized to…

astro-ph.SR2025

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…

astro-ph.SR2025★ 2 cited

Source location and evolution of a multi-lane type II radio burst

P. Zucca, P. Zhang, K. Kozarev +8

Shocks in the solar corona can accelerate electrons that in turn generate radio emission known as type II radio bursts. The characteristics and morphology of these radio bursts in…

astro-ph.SR2025★ 3 cited

Imaging and spectropolarimetric observations of a band-split type II solar radio burst with LOFAR

S. Normo, D. E. Morosan, P. Zhang +2

Type II solar radio bursts are generated by electrons accelerated by coronal shock waves. They appear in dynamic spectra as lanes drifting from higher to lower frequencies at the p…

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…