TY  -  
T1  - Observation-based modelling of magnetised coronal mass ejections with EUHFORIA 
SN  -  /  
UR  - http://hdl.handle.net/10138/321009 
T3  -  
A1  - Scolini, C.; Rodriguez, L.; Mierla, M.; Pomoell, J.; Poedts, S. 
A2  -  
PB  -  
Y1  - 2019 
LA  - eng 
AB  - Context. Coronal mass ejections (CMEs) are the primary source of strong space weather disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic pressure and internal magnetic fields, for which reliable predictions at Earth are not possible with traditional cone CME models. Aims. We study two well-observed Earth-directed CMEs using the EUropean Heliospheric FORecasting Information Asset (EUH-FORIA) model, testing for the first time the predictive capabilities of a line... 
VO  -  
IS  -  
SP  -  
OP  -  
KW  - Sun: coronal mass ejections (CMEs); Sun: heliosphere; Sun: magnetic fields; solar-terrestrial relations; solar wind; magnetohydrodynamics (MHD); SOLAR-CYCLE 23; ARRIVAL-TIME; CMES; EVOLUTION; CLOUD; GEOEFFECTIVENESS; PROPAGATION; INSTRUMENT; EXPANSION; MESSENGER; 115 Astronomy, Space science 
N1  -   
PP  -  
ER  -