146 citations · 468 across the 21 of their papers we have counts for
7 papers · 1 filter
3D propagation of relativistic solar protons through interplanetary space
S. Dalla, G. De Nolfo, A. Bruno +5
Context. Solar Energetic Particles (SEPs) with energy in the GeV range can propagate to Earth from their acceleration region near the Sun and produce Ground Level Enhancements (GLE…
Comprehensive Characterization of Solar Eruptions With Remote and In-Situ Observations, and Modeling: The Major Solar Events on 4 November 2015
Iver H. Cairns, Kamen A. Kozarev, Nariaki V. Nitta +12
Solar energetic particles (SEPs) are an important product of solar activity. They are connected to solar active regions and flares, coronal mass ejections (CMEs), EUV waves, shocks…
Modelling of proton acceleration in application to a ground level enhancement
A. Afanasiev, R. Vainio, A. P. Rouillard +3
The source of high-energy protons (>500 MeV) responsible for the so-called ground level enhancements (GLEs) remains an open question in solar physics. One of the candidates is a sh…
Injection of thermal and suprathermal seed particles into coronal shocks of varying obliquity
Markus Battarbee, Rami Vainio, Timo Laitinen +1
Context: Diffusive shock acceleration in the solar corona can accelerate solar energetic particles to very high energies. Acceleration efficiency is increased by entrapment through…
Particle scattering in turbulent plasmas with amplified wave modes
Sebastian Lange, Felix Spanier, Markus Battarbee +2
High-energy particles stream during coronal mass ejections or flares through the plasma of the solar wind. This causes instabilities, which lead to wave growth at specific resonant…
Heavy-ion Acceleration and Self-generated Waves in Coronal Shocks
Markus Battarbee, Timo Laitinen, Rami Vainio
Context: Acceleration in coronal mass ejection driven shocks is currently considered the primary source of large solar energetic particle events. Aims: The solar wind, which feeds…