The Chinese Hα solar explorer (CHASE) mission: an overview
Abstract The Chinese Hα Solar Explorer (CHASE), dubbed “Xihe”—Goddess of the Sun,
was launched on October 14, 2021 as the first solar space mission of China National Space …
was launched on October 14, 2021 as the first solar space mission of China National Space …
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 …
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 …
Data-constrained Magnetohydrodynamic Simulation of an Intermediate Solar Filament Eruption
Solar eruptive activities could occur in weak magnetic field environments and over large
spatial scales, which are especially relevant to eruptions involving intermediate or quiescent …
spatial scales, which are especially relevant to eruptions involving intermediate or quiescent …
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 …
Decoding the pre-eruptive magnetic field configurations of coronal mass ejections
A clear understanding of the nature of the pre-eruptive magnetic field configurations of
Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting …
Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting …
Modelling a multi-spacecraft coronal mass ejection encounter with EUHFORIA
E Asvestari, J Pomoell, E Kilpua, S Good… - Astronomy & …, 2021 - aanda.org
Context. Coronal mass ejections (CMEs) are a manifestation of the Sun's eruptive nature.
They can have a great impact on Earth, but also on human activity in space and on the …
They can have a great impact on Earth, but also on human activity in space and on the …
Origin and structures of solar eruptions II: Magnetic modeling
The topology and dynamics of the three-dimensional magnetic field in the solar atmosphere
govern various solar eruptive phenomena and activities, such as flares, coronal mass …
govern various solar eruptive phenomena and activities, such as flares, coronal mass …
Simulations of solar filament fine structures and their counterstreaming flows
Solar filaments, also called solar prominences when appearing above the solar limb, are
cold, dense materials suspended in the hot tenuous solar corona, consisting of numerous …
cold, dense materials suspended in the hot tenuous solar corona, consisting of numerous …
Three-dimensional MHD simulations of solar prominence oscillations in a magnetic flux rope
Solar prominences are subject to all kinds of perturbations during their lifetime, and
frequently demonstrate oscillations. The study of prominence oscillations provides an …
frequently demonstrate oscillations. The study of prominence oscillations provides an …