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Coronal mass ejections and their sheath regions in interplanetary space
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 …
originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a …
CME Theory and Models: Report of Working Group D
This chapter provides an overview of current efforts in the theory and modeling of CMEs.
Five key areas are discussed:(1) CME initiation;(2) CME evolution and propagation;(3) the …
Five key areas are discussed:(1) CME initiation;(2) CME evolution and propagation;(3) the …
On the mesoscale structure of coronal mass ejections at Mercury's orbit: BepiColombo and Parker Solar Probe observations
On 2022 February 15, an impressive filament eruption was observed off the solar eastern
limb from three remote-sensing viewpoints, namely, Earth, STEREO-A, and Solar Orbiter. In …
limb from three remote-sensing viewpoints, namely, Earth, STEREO-A, and Solar Orbiter. In …
Understanding the Internal Magnetic Field Configurations of ICMEs Using More than 20 Years of Wind Observations
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 …
interplanetary coronal mass ejections (ICMEs) are not yet fully and consistently described by …
Earth-affecting solar transients: a review of progresses in solar cycle 24
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 …
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …
On the magnetic flux budget in low-corona magnetic reconnection and interplanetary coronal mass ejections
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 …
the low corona in the wake of coronal mass ejections (CMEs) and the magnetic flux in …
Sun-to-Earth MHD simulation of the 2000 July 14 “Bastille Day” eruption
Solar eruptions are the main driver of space-weather disturbances at Earth. Extreme events
are of particular interest, not only because of the scientific challenges they pose, but also …
are of particular interest, not only because of the scientific challenges they pose, but also …
Rotation and interaction of the CMEs of September 8 and 10, 2014, tested with EUHFORIA
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 …
CMEs and solar wind structures to undergo rotation and deflection during their propagation …
Statistical study of magnetic cloud erosion by magnetic reconnection
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 …
amounts of the outer magnetic flux of interplanetary magnetic clouds (MCs) as they …
A summary of WIND magnetic clouds for years 1995-2003: model-fitted parameters, associated errors and classifications
RP Lep**, DB Berdichevsky, CC Wu… - Annales …, 2006 - angeo.copernicus.org
Interplanetary magnetic clouds (MCs) have been identified for the first 8.6 years of the WIND
mission, and their magnetic field structures have been parameter-fitted by a static, force free …
mission, and their magnetic field structures have been parameter-fitted by a static, force free …