activity
20142026
most citedMultiple Regions of Shock-accelerated Particles during a Solar Coronal Mass Ejection

89 citations · 861 across the 43 of their papers we have counts for

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Showing 2020Show all

5 papers · 1 filter

astro-ph.SR2020★ 24 cited

On the occurrence of type IV solar radio bursts in the solar cycle 24 and their association with coronal mass ejections

Anshu Kumari, D. E. Morosan, E. K. J. Kilpua

Solar activity, in particular coronal mass ejections (CMEs), are often accompanied by bursts of radiation at metre wavelengths. Some of these bursts have a long duration and extend…

astro-ph.SR2020★ 10 cited

Electron acceleration and radio emission following the early interaction of two coronal mass ejections

D. E. Morosan, E. Palmerio, J. E. Räsänen +6

Context. Coronal mass ejections (CMEs) are large eruptions of magnetised plasma from the Sun that are often accompanied by solar radio bursts produced by accelerated electrons. Aim…

astro-ph.SR2020★ 22 cited

Interferometric Imaging with LOFAR Remote Baselines of the Fine Structures of a Solar Type IIIb Radio Burst

PeiJin Zhang, Pietro Zucca, Sarrvesh Seethapuram Sridhar +8

Context. Solar radio bursts originate mainly from high energy electrons accelerated in solar eruptions like solar flares, jets, and coronal mass ejections. A subcategory of solar r…

astro-ph.SR2020★ 5 cited

The frequency drift and fine structures of Solar S-bursts in the high frequency band of LOFAR

PeiJin Zhang, Pietro Zucca, ChuanBing Wang +8

Solar S-bursts are short duration ( s at decameter wavelengths) radio bursts that have been observed during periods of moderate solar activity, where S stands for short. The fr…

astro-ph.SR2020★ 18 cited

Three-dimensional reconstruction of multiple particle acceleration regions during a coronal mass ejection

D. E. Morosan, E. Palmerio, J. Pomoell +3

Context. Some of the most prominent sources for particle acceleration in our Solar System are large eruptions of magnetised plasma from the Sun called coronal mass ejections (CMEs)…