[HTML][HTML] Coronal mass ejections: Observations
DF Webb, TA Howard - Living Reviews in Solar Physics, 2012 - Springer
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 …
particles, and radio bursts. Since the vast majority of these are associated with the eruption …
The physical processes of CME/ICME evolution
W Manchester, EKJ Kilpua, YD Liu, N Lugaz… - Space Science …, 2017 - Springer
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 …
Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections
YD Liu, JG Luhmann, P Kajdič, EKJ Kilpua… - Nature …, 2014 - nature.com
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 …
Origin and structures of solar eruptions I: magnetic flux rope
Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic
eruptive phenomena in our solar system and able to release a large quantity of plasma and …
eruptive phenomena in our solar system and able to release a large quantity of plasma and …
Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU
Forecasting the in situ properties of coronal mass ejections (CMEs) from remote images is
expected to strongly enhance predictions of space weather and is of general interest for …
expected to strongly enhance predictions of space weather and is of general interest for …
The first super geomagnetic storm of solar cycle 24:“The St. Patrick's day event (17 March 2015)”
CC Wu, K Liou, RP Lepping, L Hutting, S Plunkett… - Earth, Planets and …, 2016 - Springer
The first super geomagnetic storm (Dst<− 200 nT) of solar cycle 24 occurred on “St. Patrick's
day”(17 March 2015). Notably, it was a two-step storm. The source of the storm can be …
day”(17 March 2015). Notably, it was a two-step storm. The source of the storm can be …
On Sun-to-Earth propagation of coronal mass ejections
We investigate how coronal mass ejections (CMEs) propagate through, and interact with, the
inner heliosphere between the Sun and Earth, a key question in CME research and space …
inner heliosphere between the Sun and Earth, a key question in CME research and space …
STEREO observations of interplanetary coronal mass ejections in 2007–2016
LK Jian, CT Russell, JG Luhmann… - The Astrophysical …, 2018 - iopscience.iop.org
We have conducted a survey of 341 interplanetary coronal mass ejections (ICMEs) using
STEREO A/B data, analyzing their properties while extending a Level 3 product through …
STEREO A/B data, analyzing their properties while extending a Level 3 product through …
Multi-point shock and flux rope analysis of multiple interplanetary coronal mass ejections around 2010 August 1 in the inner heliosphere
We present multi-point in situ observations of a complex sequence of coronal mass ejections
(CMEs) which may serve as a benchmark event for numerical and empirical space weather …
(CMEs) which may serve as a benchmark event for numerical and empirical space weather …
Flare-CME models: an observational perspective (invited review)
B Schmieder, G Aulanier, B Vršnak - Solar physics, 2015 - Springer
Eruptions, flares, and coronal mass ejection (CMEs) are due to physical phenomena mainly
driven by an initially force-free current-carrying magnetic field. We review some key …
driven by an initially force-free current-carrying magnetic field. We review some key …