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 …
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 …
Coronal mass ejections over solar cycles 23 and 24
PL Lamy, O Floyd, B Boclet, J Wojak, H Gilardy… - Space Science …, 2019 - Springer
We present a statistical analysis of solar coronal mass ejections (CMEs) based on 23 years
of quasi-continuous observations with the LASCO coronagraph, thus covering two complete …
of quasi-continuous observations with the LASCO coronagraph, thus covering two complete …
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 …
A comprehensive three-dimensional radiative magnetohydrodynamic simulation of a solar flare
MCM Cheung, M Rempel, G Chintzoglou, F Chen… - Nature …, 2019 - nature.com
Solar and stellar flares are the most intense emitters of X-rays and extreme ultraviolet
radiation in planetary systems,. On the Sun, strong flares are usually found in newly …
radiation in planetary systems,. On the Sun, strong flares are usually found in newly …
Magnetic flux ropes in the solar corona: structure and evolution toward eruption
R Liu - Research in Astronomy and Astrophysics, 2020 - iopscience.iop.org
Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …
A model for confined solar eruptions including external reconnection
J Chen, X Cheng, B Kliem… - The Astrophysical Journal …, 2023 - iopscience.iop.org
The violent disruption of the coronal magnetic field is often observed to be restricted to the
low corona, appearing as a confined eruption. The possible causes of the confinement …
low corona, appearing as a confined eruption. The possible causes of the confinement …
Chromosphere to 1 AU simulation of the 2011 March 7th event: a comprehensive study of coronal mass ejection propagation
We perform and analyze the results of a global magnetohydrodynamic simulation of the fast
coronal mass ejection (CME) that occurred on 2011 March 7. The simulation is made using …
coronal mass ejection (CME) that occurred on 2011 March 7. The simulation is made using …
Deciphering the slow-rise precursor of a major coronal mass ejection
Coronal mass ejections are explosive plasma phenomena prevalently occurring on the Sun
and probably on other magnetically active stars. However, how their pre-eruptive …
and probably on other magnetically active stars. However, how their pre-eruptive …
The source and engine of coronal mass ejections
MK Georgoulis, A Nindos… - … Transactions of the …, 2019 - royalsocietypublishing.org
Coronal mass ejections (CMEs) are large-scale expulsions of coronal plasma and magnetic
field propagating through the heliosphere. Because CMEs are observed by white-light …
field propagating through the heliosphere. Because CMEs are observed by white-light …