298 citations · 3k across the 98 of their papers we have counts for
12 papers · 1 filter
Extended radio emission associated with a breakout eruption from the back side of the Sun
D. E. Morosan, E. Palmerio, B. J. Lynch +1
Context. Coronal mass ejections (CMEs) on the Sun are the largest explosions in the Solar System that can drive powerful plasma shocks. The eruptions, shocks, and other processes a…
CME-CME Interactions as Sources of CME Geo-effectiveness: The Formation of the Complex Ejecta and Intense Geomagnetic Storm in Early September 2017
Camilla Scolini, Emmanuel Chané, Manuela Temmer +9
Coronal mass ejections (CMEs) are the primary sources of intense disturbances at Earth, where their geo-effectiveness is largely determined by their dynamic pressure and internal m…
In situ measurements of the variable slow solar wind near sector boundaries
E. Sanchez-Diaz, A. Rouillard, B. Lavraud +2
The release of density structures at the tip of the coronal helmet streamers, likely as a consequence of magnetic reconnection, contributes to the mass flux of the slow solar wind.…
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…
Multiple Regions of Shock-accelerated Particles during a Solar Coronal Mass Ejection
Diana E. Morosan, Eoin P. Carley, Laura A. Hayes +8
The Sun is an active star that can launch large eruptions of magnetised plasma into the heliosphere, called coronal mass ejections (CMEs). These ejections can drive shocks that acc…
Testing the background solar wind modelled by EUHFORIA
J. Hinterreiter, J. Magdalenic, M. Temmer +10
In order to address the growing need for more accurate space weather predictions, a new model named EUHFORIA (EUropean Heliospheric FORecasting Information Asset) was recently deve…