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A fundamental mechanism of solar eruption initiation
Solar eruptions are spectacular magnetic explosions in the Sun's corona, and how they are
initiated remains unclear. Prevailing theories often rely on special magnetic topologies that …
initiated remains unclear. Prevailing theories often rely on special magnetic topologies that …
Developments of a fundamental mechanism for initiation of solar eruptions
Solar eruptions are outbursts of magnetized plasma in the atmosphere of the Sun,
encompassing phenomena like solar flares, ejective prominences and coronal mass …
encompassing phenomena like solar flares, ejective prominences and coronal mass …
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 …
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-driven modeling of a coronal magnetic flux rope: from birth to death
Magnetic flux ropes are a bundle of twisted magnetic field lines produced by internal electric
currents, which are responsible for solar eruptions and are the major drivers of geomagnetic …
currents, which are responsible for solar eruptions and are the major drivers of geomagnetic …
Characteristics and applications of interplanetary coronal mass ejection composition
HQ Song, S Yao - Science China Technological Sciences, 2020 - Springer
In situ measurements of interplanetary coronal mass ejection (ICME) composition, including
elemental abundances and charge states of heavy ions, open a new avenue to study …
elemental abundances and charge states of heavy ions, open a new avenue to study …
Eruption of a multi-flux-rope system in solar active region 12673 leading to the two largest flares in Solar Cycle 24
YJ Hou, J Zhang, T Li, SH Yang, XH Li - Astronomy & Astrophysics, 2018 - aanda.org
Context. Solar active region (AR) 12673 in 2017 September produced the two largest flares
in Solar Cycle 24: the X9. 3 flare on September 6 and the X8. 2 flare on September 10. Aims …
in Solar Cycle 24: the X9. 3 flare on September 6 and the X8. 2 flare on September 10. Aims …
Understanding the twist distribution inside magnetic flux ropes by anatomizing an interplanetary magnetic cloud
Magnetic flux rope (MFR) is the core structure of the greatest eruptions, that is, the coronal
mass ejections (CMEs), on the Sun, and magnetic clouds are posteruption MFRs in …
mass ejections (CMEs), on the Sun, and magnetic clouds are posteruption MFRs in …
Modeling the propagation of coronal mass ejections with COCONUT: Implementation of the regularized Biot-Savart law flux rope model
Context. Coronal mass ejections (CMEs) are rapid eruptions of magnetized plasma that
occur on the Sun. They are known to be the main drivers of adverse space weather. The …
occur on the Sun. They are known to be the main drivers of adverse space weather. The …
Magnetohydrodynamic modeling of a solar eruption associated with an X9. 3 flare observed in the active region 12673
On 2017 September 6, the solar active region 12673 produced an X9. 3 flare, regarded to be
the largest to have occurred in solar cycle 24. In this work we have performed a …
the largest to have occurred in solar cycle 24. In this work we have performed a …