This review article summarizes the advancement in the studies of Earth-affecting solar
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …

As observed in Thomson-scattered white light, coronal mass ejections (CMEs) are manifest
as large-scale expulsions of plasma magnetically driven from the corona in the most …

The magnetic topology, structure, and geometry of the magnetic obstacles embedded within
interplanetary coronal mass ejections (ICMEs) are not yet fully and consistently described by …

We present the first quantitative comparison between the total magnetic reconnection flux in
the low corona in the wake of coronal mass ejections (CMEs) and the magnetic flux in …

During propagation, Magnetic Clouds (MC) interact with their environment and, in particular,
may reconnect with the solar wind around it, eroding away part of its initial magnetic flux …

Several recent studies suggest that magnetic reconnection is able to erode substantial
amounts of the outer magnetic flux of interplanetary magnetic clouds (MCs) as they …

We study interplanetary coronal mass ejections (ICMEs) measured by probes at different
heliocentric distances (0.3–1 AU) to investigate the propagation of ICMEs in the inner …

Much progress has been made in the study of coronal mass ejections (CMEs), the main
drivers of terrestrial space weather thanks to the deployment of several missions in the last …

Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …

The solar wind conditions at one astronomical unit (AU) can be strongly disturbed by
interplanetary coronal mass ejections (ICMEs). A subset, called magnetic clouds (MCs), is …