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

collaborators

7 papers

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…

physics.space-ph2019★ 5 cited

Kappa-Maxwellian electrons and Bi-Maxwellian protons in a two-fluid model for fast solar wind

Somayeh Taran, Hossein Safari, Farhad Daei

Modeling fast solar wind based on the kinetic theory is an important task for scientists. In this paper, we present a two-fluid model for fast solar wind with anisotropic Kappa-Max…