Solar eruptive phenomena embrace a variety of eruptions, including flares, solar energetic
particles, and radio bursts. Since the vast majority of these are associated with the eruption …

We present a statistical analysis of solar coronal mass ejections (CMEs) based on 23 years
of quasi-continuous observations with the LASCO coronagraph, thus covering two complete …

Solar coronal mass ejections (CMEs) are the most significant drivers of adverse space
weather on Earth, but the physics governing their propagation through the heliosphere is not …

In Fall 2008 NASA selected a large international consortium to produce a comprehensive
automated feature-recognition system for the Solar Dynamics Observatory (SDO). The SDO …

In this Letter, we present the first direct detection of a rotating coronal mass ejection (CME) in
the middle corona (5–15 R☉). The CME rotation rate is 60 day–1, which is the highest rate …

This review presents a comprehensive and systematic overview of image-processing
techniques that are used in automated feature-detection algorithms applied to solar data: i) …

Automated techniques for detecting and tracking coronal mass ejections (CMEs) in
coronagraph data are of ever increasing importance for space weather monitoring and …

Studying coronal mass ejections (CMEs) in coronagraph data can be challenging due to
their diffuse structure and transient nature, and user-specific biases may be introduced …

Context. In the scope of space weather forecasting, it is crucial to be able to more reliably
predict the arrival time, speed, and magnetic field configuration of coronal mass ejections …

Context. The configuration of the interplanetary magnetic field and features of the related
ambient solar wind in the ecliptic and meridional plane are different. Therefore, one can …