activity
20192025
most citedType II radio bursts and their association with coronal mass ejections in solar cycles 23 and 24

35 citations · 65 across the 7 of their papers we have counts for

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Showing astro-ph.SRShow all

6 papers · 1 filter

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.SR2024★ 3 cited

The effect of data-driving and relaxation model on magnetic flux rope evolution and stability

Andreas Wagner, Daniel J. Price, Slava Bourgeois +7

We investigate the effect of data-driving on flux rope eruptivity in magnetic field simulations by analysing fully data-driven modelling results of active region (AR) 12473 and AR1…

astro-ph.SR2023★ 8 cited

The Automatic Identification and Tracking of Coronal Flux Ropes -- Part I: Footpoints and Fluxes

Andreas Wagner, Emilia K. J. Kilpua, Ranadeep Sarkar +5

Investigating the early-stage evolution of an erupting flux rope from the Sun is important to understand the mechanisms of how it looses its stability and its space weather impacts…

astro-ph.SR2023★ 35 cited

Type II radio bursts and their association with coronal mass ejections in solar cycles 23 and 24

Anshu Kumari, Diana E. Morosan, E. K. J. Kilpua +1

Metre wavelength type II solar radio bursts are believed to be the signatures of shock-accelerated electrons in the corona. Studying these bursts can give information about the ini…

astro-ph.SR2023★ 5 cited

Effects of optimisation parameters on data-driven magnetofrictional modelling of active regions

A. Kumari, D. J. Price, F. Daei +2

Data-driven time-dependent magnetofrictional modelling (TMFM) of active region magnetic fields has been proven to be a useful tool to study the corona. The input to the model is th…

astro-ph.SR2022★ 9 cited

Flux-tube-dependent propagation of Alfvén waves in the solar corona

Chaitanya Prasad Sishtla, Jens Pomoell, Emilia Kilpua +3

Alfvén-wave turbulence has emerged as an important heating mechanism to accelerate the solar wind. The generation of this turbulent heating is dependent on the presence and subsequ…