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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 …
The physical processes of CME/ICME evolution
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 …
as large-scale expulsions of plasma magnetically driven from the corona in the most …
The Plasma and Suprathermal Ion Composition (PLASTIC) investigation on the STEREO observatories
Abstract The Plasma and Suprathermal Ion Composition (PLASTIC) investigation provides
the in situ solar wind and low energy heliospheric ion measurements for the NASA Solar …
the in situ solar wind and low energy heliospheric ion measurements for the NASA Solar …
Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections
Abstract Space weather refers to dynamic conditions on the Sun and in the space
environment of the Earth, which are often driven by solar eruptions and their subsequent …
environment of the Earth, which are often driven by solar eruptions and their subsequent …
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 …
A Quarter Century of Wind Spacecraft Discoveries
LB Wilson III, AL Brosius, N Gopalswamy… - 2021 - Wiley Online Library
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 …
Heliophysics System Observatory (HSO)—a fleet of spacecraft created to understand the …
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 …
Kinematic treatment of coronal mass ejection evolution in the solar wind
P Riley, NU Crooker - The Astrophysical Journal, 2004 - iopscience.iop.org
We present a kinematic study of the evolution of coronal mass ejections (CMEs) in the solar
wind. Specifically, we consider the effects of (1) spherical expansion and (2) uniform …
wind. Specifically, we consider the effects of (1) spherical expansion and (2) uniform …
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 …
Statistical study of the interplanetary coronal mass ejections from 1995 to 2015
We establish a catalog of interplanetary coronal mass ejections (ICMEs) during the period
from 1995 to 2015 using the in-situ observations from the Wind and ACE spacecraft. Based …
from 1995 to 2015 using the in-situ observations from the Wind and ACE spacecraft. Based …