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 …
Some interesting topics provoked by the solar filament research in the past decade
Solar filaments are an intriguing phenomenon, like cool clouds suspended in the hot corona.
Similar structures exist in the intergalactic medium as well. Despite being a long-studied …
Similar structures exist in the intergalactic medium as well. Despite being a long-studied …
Minifilament eruptions that drive coronal jets in a solar active region
AC Sterling, RL Moore, DA Falconer… - The Astrophysical …, 2016 - iopscience.iop.org
We present observations of eruptive events in an active region adjacent to an on-disk
coronal hole on 2012 June 30, primarily using data from the Solar Dynamics Observatory …
coronal hole on 2012 June 30, primarily using data from the Solar Dynamics Observatory …
Chirality and magnetic configurations of solar filaments
It has been revealed that the magnetic topology in the solar atmosphere displays
hemispheric preference, ie, helicity is mainly negative/positive in the northern/southern …
hemispheric preference, ie, helicity is mainly negative/positive in the northern/southern …
Magnetic twists of solar filaments
JH Guo, YW Ni, Y Qiu, Z Zhong, Y Guo… - The Astrophysical …, 2021 - iopscience.iop.org
Solar filaments are cold and dense materials situated in magnetic dips, which show distinct
radiation characteristics compared to the surrounding coronal plasma. They are associated …
radiation characteristics compared to the surrounding coronal plasma. They are associated …
Witnessing tether-cutting reconnection at the onset of a partial eruption
In this paper, we study the onset process of a solar eruption on 2015 February 21, focusing
on its unambiguous precursor phase. With multiwavelength imaging observations from the …
on its unambiguous precursor phase. With multiwavelength imaging observations from the …
Initiation and early kinematic evolution of solar eruptions
We investigate the initiation and early evolution of 12 solar eruptions, including six active-
region hot channel and six quiescent filament eruptions, which were well observed by the …
region hot channel and six quiescent filament eruptions, which were well observed by the …
Toward a unified explanation for the three-part structure of solar coronal mass ejections
H Song, L Li, Y Chen - The Astrophysical Journal, 2022 - iopscience.iop.org
Coronal mass ejections (CMEs) are associated with the eruption of magnetic flux ropes
(MFRs), which usually appear as hot channels in active regions and coronal cavities in quiet …
(MFRs), which usually appear as hot channels in active regions and coronal cavities in quiet …
Thermodynamic and magnetic topology evolution of the X1. 0 Flare on 2021 October 28 simulated by a data-driven radiative magnetohydrodynamic model
JH Guo, YW Ni, Z Zhong, Y Guo, C **a… - The Astrophysical …, 2023 - iopscience.iop.org
Solar filament eruptions, flares, and coronal mass ejections (CMEs) are manifestations of
drastic releases of energy in the magnetic field, which are related to many eruptive …
drastic releases of energy in the magnetic field, which are related to many eruptive …
Comparison of the Composition of ICMEs from Active Regions and Quiet-Sun Regions
The composition of interplanetary coronal mass ejections (ICMEs), including the ionic
charge states and elemental abundances of heavy elements, is tightly correlated with their …
charge states and elemental abundances of heavy elements, is tightly correlated with their …