Coronal mass ejections and their sheath regions in interplanetary space
E Kilpua, HEJ Koskinen, TI Pulkkinen - Living Reviews in Solar Physics, 2017 - Springer
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 …
[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 soho/lasco cme catalog
N Gopalswamy, S Yashiro, G Michalek… - Earth, Moon, and …, 2009 - Springer
Coronal mass ejections (CMEs) are routinely identified in the images of the solar corona
obtained by the Solar and Heliospheric Observatory (SOHO) mission's Large Angle and …
obtained by the Solar and Heliospheric Observatory (SOHO) mission's Large Angle and …
CME–CME interactions as sources of CME geoeffectiveness: The formation of the complex ejecta and intense geomagnetic storm in 2017 early September
Coronal mass ejections (CMEs) are the primary sources of intense disturbances at Earth,
where their geoeffectiveness is largely determined by their dynamic pressure and internal …
where their geoeffectiveness is largely determined by their dynamic pressure and internal …
Properties of ground level enhancement events and the associated solar eruptions during solar cycle 23
N Gopalswamy, H Xie, S Yashiro, S Akiyama… - Space Science …, 2012 - Springer
Solar cycle 23 witnessed the most complete set of observations of coronal mass ejections
(CMEs) associated with the Ground Level Enhancement (GLE) events. We present an …
(CMEs) associated with the Ground Level Enhancement (GLE) events. We present an …
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 …
Structure, stability, and evolution of magnetic flux ropes from the perspective of magnetic twist
We investigate the evolution of NOAA Active Region (AR) 11817 during 2013 August 10–12,
when it developed a complex field configuration and produced four confined, followed by …
when it developed a complex field configuration and produced four confined, followed by …
The standard flare model in three dimensions-I. Strong-to-weak shear transition in post-flare loops
G Aulanier, M Janvier, B Schmieder - Astronomy & Astrophysics, 2012 - aanda.org
Context. The standard CSHKP model for eruptive flares is two-dimensional. Yet
observational interpretations of photospheric currents in pre-eruptive sigmoids, shear in post …
observational interpretations of photospheric currents in pre-eruptive sigmoids, shear in post …
The origin, early evolution and predictability of solar eruptions
Coronal mass ejections (CMEs) were discovered in the early 1970s when space-borne
coronagraphs revealed that eruptions of plasma are ejected from the Sun. Today, it is known …
coronagraphs revealed that eruptions of plasma are ejected from the Sun. Today, it is known …
Suppression of coronal mass ejections in active stars by an overlying large-scale magnetic field: a numerical study
JD Alvarado-Gómez, JJ Drake, O Cohen… - The Astrophysical …, 2018 - iopscience.iop.org
We present results from a set of numerical simulations aimed at exploring the mechanism of
coronal mass ejection (CME) suppression in active stars by an overlying large-scale …
coronal mass ejection (CME) suppression in active stars by an overlying large-scale …