Solar eruptions, observed as flares and coronal mass ejections (CMEs), are the most
energetic visible plasma phenomena in the solar system. CMEs are the central component …

Eruptions, flares, and coronal mass ejection (CMEs) are due to physical phenomena mainly
driven by an initially force-free current-carrying magnetic field. We review some key …

We present a forward-modeling technique for flux rope-like CMEs using an empirically
defined model of a flux rope, the graduated cylindrical shell (GCS). To compare it with white …

The graduated cylindrical shell (GCS) model developed by Thernisien et al. has been used
with the goal of studying the three-dimensional morphology, position, and kinematics of …

Magnetic flux ropes play a central role in the physics of coronal mass ejections (CMEs).
Although a flux-rope topology is inferred for the majority of coronagraphic observations of …

Solar coronal mass ejections (CMEs) show a large variety in their kinematic properties.
CMEs originating in active regions and accompanied by strong flares are usually faster and …

Flux ropes are now generally accepted to be the magnetic configuration of coronal mass
ejections (CMEs), which may be formed prior to or during solar eruptions. In this study, we …

The most important observational characteristics of coronal mass ejections (CMEs) are
summarized, emphasizing those aspects which are relevant for testing physical concepts …

We study kinematics of 22 coronal mass ejections (CMEs) whose motion was traced from
the gradual pre-acceleration phase up to the post-acceleration stage. The peak …

Coronal mass ejections (CMEs) are the primary drivers of severe space weather
disturbances in the heliosphere. Models of CME dynamics have been proposed that do not …