89 citations · 861 across the 43 of their papers we have counts for
5 papers · 1 filter
Connecting remote and in situ observations of shock-accelerated electrons associated with a coronal mass ejection
D. E. Morosan, J. Pomoell, C. Palmroos +7
One of the most prominent sources for energetic particles in our solar system are huge eruptions of magnetised plasma from the Sun called coronal mass ejections (CMEs), which usual…
Spatially resolved radio signatures of electron beams in a coronal shock
Peijin Zhang, Diana Morosan, Anshu Kumari +1
Context. Type II radio bursts are solar radio burst associated with coronal shocks. Type II bursts usually exhibit fine structures in dynamic spectra that represent signatures of a…
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…
A type II solar radio burst without a coronal mass ejection
D. E. Morosan, J. Pomoell, A. Kumari +2
The Sun produces the most powerful explosions in the solar system, solar flares, that can also be accompanied by large eruptions of magnetised plasma, coronal mass ejections (CMEs)…
On the Role of Interplanetary Shocks in Accelerating MeV Electrons
N. Talebpour Sheshvan, N. Dresing, R. Vainio +2
One of the sources of solar energetic particle (SEP) events is shocks that are driven by fast coronal mass ejections (CMEs). They can accelerate SEPs up to relativistic energies an…