Interplanetary coronal mass ejections (ICMEs) are large-scale heliospheric transients that
originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a …

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 …

During the thirteenth encounter of the Parker Solar Probe (PSP) mission, the spacecraft
traveled through a topologically complex interplanetary coronal mass ejection (ICME) …

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 …

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 Wind spacecraft, launched on November 1, 1994, is a critical element in NASA's
Heliophysics System Observatory (HSO)—a fleet of spacecraft created to understand the …

Magnetic reconnection in current sheets converts magnetic energy into particle energy. The
process may play an important role in the acceleration and heating of the solar wind close to …

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 explore the role of heliospheric magnetic field configurations and conditions that favor
the generation and confinement of small-scale magnetic islands associated with atypical …

We report observations of reconnection exhausts in the Heliospheric Current Sheet (HCS)
during Parker Solar Probe Encounters 08 and 07, at 16 Rs and 20 Rs, respectively …