130 citations · 1.8k across the 51 of their papers we have counts for
52 papers
Three-dimensional modelling of the shock-turbulence interaction
Domenico Trotta, Oreste Pezzi, David Burgess +12
The complex interaction between shocks and plasma turbulence is extremely important to address crucial features of energy conversion in a broad range of astrophysical systems. We s…
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)…
Global energetics of solar powerful events on 6 September 2017
Dong Li, Alexander Warmuth, Jincheng Wang +9
Solar flares and coronal mass ejections (CMEs) are thought to be the most powerful events on the Sun. They can release energy as high as 10^32 erg in tens of minutes,and could prod…
Multiple injections of energetic electrons associated with the flare/CME event on 9 October 2021
Immanuel Christopher Jebaraj, Athanasios Kouloumvakos, Nina Dresing +11
We study the solar energetic particle (SEP) event observed on 9 October 2021, by multiple spacecraft including Solar Orbiter (SolO). The event was associated with an M1.6 flare, a…
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…
Shock-accelerated electrons during the fast expansion of a coronal mass ejection
D. E. Morosan, J. Pomoell, A. Kumari +2
Context. Some of 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)…