Radio Emission of Flares and Coronal Mass Ejections: Invited Review

A Nindos, H Aurass, KL Klein, G Trottet - Solar Physics, 2008 - Springer
We review recent progress on our understanding of radio emission from solar flares and
coronal mass ejections (CMEs) with emphasis on those aspects of the subject that help us …

A primer on focused solar energetic particle transport: basic physics and recent modelling results

J van den Berg, DT Strauss, F Effenberger - Space Science Reviews, 2020 - Springer
The basics of focused transport as applied to solar energetic particles are reviewed, paying
special attention to areas of common misconception. The micro-physics of charged particles …

Solar flares, coronal mass ejections and solar energetic particle event characteristics

A Papaioannou, I Sandberg… - Journal of Space …, 2016 - swsc-journal.org
A new catalogue of 314 solar energetic particle (SEP) events extending over a large time
span from 1984 to 2013 has been compiled. The properties as well as the associations of …

The first widespread solar energetic particle event observed by Solar Orbiter on 2020 November 29

A Kollhoff, A Kouloumvakos, D Lario, N Dresing… - Astronomy & …, 2021 - aanda.org
Context. On 2020 November 29, the first widespread solar energetic particle (SEP) event of
solar cycle 25 was observed at four widely separated locations in the inner (≲ 1 AU) …

The first widespread solar energetic particle event of solar cycle 25 on 2020 November 29-Shock wave properties and the wide distribution of solar energetic particles

A Kouloumvakos, RY Kwon… - Astronomy & …, 2022 - aanda.org
Context. On 2020 November 29, an eruptive event occurred in an active region located
behind the eastern solar limb as seen from Earth. The event consisted of an M4. 4 class …

The longitudinal properties of a solar energetic particle event investigated using modern solar imaging

AP Rouillard, NR Sheeley, A Tylka… - The Astrophysical …, 2012 - iopscience.iop.org
We use combined high-cadence, high-resolution, and multi-point imaging by the Solar-
Terrestrial Relations Observatory (STEREO) and the Solar and Heliospheric Observatory to …

Deriving the properties of coronal pressure fronts in 3D: application to the 2012 May 17 ground level enhancement

AP Rouillard, I Plotnikov, RF Pinto… - The Astrophysical …, 2016 - iopscience.iop.org
We study the link between an expanding coronal shock and the energetic particles
measured near Earth during the ground level enhancement of 2012 May 17. We developed …

Connecting remote and in situ observations of shock-accelerated electrons associated with a coronal mass ejection

DE Morosan, J Pomoell, C Palmroos, N Dresing… - Astronomy & …, 2024 - aanda.org
Context. One of the most prominent sources for energetic particles in our Solar System are
huge eruptions of magnetised plasma from the Sun, known as coronal mass ejections …

The first SEPServer event catalogue~ 68-MeV solar proton events observed at 1 AU in 1996–2010

R Vainio, E Valtonen, B Heber… - Journal of space …, 2013 - swsc-journal.org
SEPServer is a three-year collaborative project funded by the seventh framework
programme (FP7-SPACE) of the European Union. The objective of the project is to provide …

Irregular proton injection to high energies at interplanetary shocks

D Trotta, TS Horbury, D Lario, R Vainio… - The Astrophysical …, 2023 - iopscience.iop.org
How thermal particles are accelerated to suprathermal energies is an unsolved issue,
crucial for many astrophysical systems. We report novel observations of irregular, dispersive …