34 citations · 124 across the 5 of their papers we have counts for
9 papers
Flux-tube-dependent propagation of Alfvén waves in the solar corona
Chaitanya Prasad Sishtla, Jens Pomoell, Emilia Kilpua +3
Alfvén-wave turbulence has emerged as an important heating mechanism to accelerate the solar wind. The generation of this turbulent heating is dependent on the presence and subsequ…
ULF wave transmission across collisionless shocks: 2.5D local hybrid simulations
Primoz Kajdic, Yann Pfau-Kempf, Lucile Turc +10
We study the interaction of upstream ultra-low frequency (ULF) waves with collisionless shocks by analyzing the outputs of eleven 2D local hybrid simulation runs. Our simulated sho…
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…
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)…
Particle Telescope aboard FORESAIL-1: simulated performance
Philipp Oleynik, Rami Vainio, Hannu-Pekka Hedman +18
The Particle Telescope (PATE) of FORESAIL-1 mission is described. FORESAIL-1 is a CubeSat mission to polar Low Earth Orbit. Its scientific objectives are to characterize electron p…
Exploring Solar-Terrestrial Interactions via Multiple Observers (A White Paper for the Voyage 2050 long-term plan in the ESA Science Programme)
G. Branduardi-Raymont, M. Berthomier, Y. Bogdanova +24
This paper addresses the fundamental science question: "How does solar wind energy flow through the Earth's magnetosphere, how is it converted and distributed?". We need to underst…