[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 …
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 …
Implementation of the graduated cylindrical shell model for the three-dimensional reconstruction of coronal mass ejections
A Thernisien - The Astrophysical Journal Supplement Series, 2011 - iopscience.iop.org
The graduated cylindrical shell (GCS) model developed by Thernisien et al. has been used
with the goal of studying the three-dimensional morphology, position, and kinematics of …
with the goal of studying the three-dimensional morphology, position, and kinematics of …
Space weather: The solar perspective: An update to Schwenn (2006)
M Temmer - Living Reviews in Solar Physics, 2021 - Springer
The Sun, as an active star, is the driver of energetic phenomena that structure interplanetary
space and affect planetary atmospheres. The effects of Space Weather on Earth and the …
space and affect planetary atmospheres. The effects of Space Weather on Earth and the …
Solar prominences: theory and models: Fleshing out the magnetic skeleton
SE Gibson - Living reviews in solar physics, 2018 - Springer
Magnetic fields suspend the relatively cool material of solar prominences in an otherwise hot
corona. A comprehensive understanding of solar prominences ultimately requires complex …
corona. A comprehensive understanding of solar prominences ultimately requires complex …
Direct evidence for a fast coronal mass ejection driven by the prior formation and subsequent destabilization of a magnetic flux rope
S Patsourakos, A Vourlidas… - The Astrophysical …, 2013 - iopscience.iop.org
Magnetic flux ropes play a central role in the physics of coronal mass ejections (CMEs).
Although a flux-rope topology is inferred for the majority of coronagraphic observations of …
Although a flux-rope topology is inferred for the majority of coronagraphic observations of …
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 …
[HTML][HTML] Large-scale globally propagating coronal waves
A Warmuth - Living Reviews in Solar Physics, 2015 - Springer
Large-scale, globally propagating wave-like disturbances have been observed in the solar
chromosphere and by inference in the corona since the 1960s. However, detailed analysis …
chromosphere and by inference in the corona since the 1960s. However, detailed analysis …
On the Nature and Genesis of EUV Waves: A Synthesis of Observations from SOHO, STEREO, SDO, and Hinode (Invited Review)
S Patsourakos, A Vourlidas - Solar Physics, 2012 - Springer
A major, albeit serendipitous, discovery of the SOlar and Heliospheric Observatory mission
was the observation by the Extreme Ultraviolet Telescope (EIT) of large-scale extreme …
was the observation by the Extreme Ultraviolet Telescope (EIT) of large-scale extreme …
Magnetic structure and propagation of two interacting CMEs from the Sun to Saturn
E Palmerio, T Nieves‐Chinchilla… - Journal of …, 2021 - Wiley Online Library
One of the grand challenges in heliophysics is the characterization of coronal mass ejection
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …
(CME) magnetic structure and evolution from eruption at the Sun through heliospheric …