Context. Solar coronal mass ejections (CMEs) can catch up and interact with preceding
CMEs and solar wind structures to undergo rotation and deflection during their propagation …

We present observations and modeling results of the propagation and impact at Earth of a
high-latitude, extended filament channel eruption that commenced on 2015 July 9. The …

Coronal mass ejections (CMEs) are the largest type of eruptions on the Sun and the main
driver of severe space weather at the Earth. In this study, we implement a force-free …

Predicting the impacts of coronal mass ejections (CMEs) is a major focus of current space
weather forecasting efforts. Typically, CME properties are reconstructed from stereoscopic …

Context. The text has been edited to adhere to American English based on the spelling style
used in the text. In order to anticipate the geoeffectiveness of coronal mass ejections …

Context. EUHFORIA is a space weather forecasting tool used to predict the time of arrival
and geo-effectiveness of coronal mass ejections (CMEs). In this simulation model, magnetic …

Aims. This study utilises a modelling approach to investigate the impact of perturbed solar
wind conditions caused by multiple interplanetary coronal mass ejections (ICMEs) on the …

Context. Coronal mass ejections (CMEs) are eruptions of plasma from the Sun that travel
through interplanetary space and may encounter Earth. CMEs often enclose a magnetic flux …

Coronal mass ejections (CMEs) and high speed streams (HSSs) are large‐scale transient
structures that routinely propagate away from the Sun. Individually, they can cause space …

Filament eruptions and coronal mass ejections are physical phenomena related to magnetic
flux ropes carrying electric current. A magnetic flux rope is a key structure for solar eruptions …