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 …
Data-driven modeling of solar coronal magnetic field evolution and eruptions
Magnetic fields play a fundamental role in the structure and dynamics of the solar corona. As
they are driven by their footpoint motions on the solar surface, which transport energy from …
they are driven by their footpoint motions on the solar surface, which transport energy from …
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 …
Measurement of magnetic field and relativistic electrons along a solar flare current sheet
In the standard model of solar flares, a large-scale reconnection current sheet is postulated
to be the central engine for powering the flare energy release,–and accelerating particles …
to be the central engine for powering the flare energy release,–and accelerating particles …
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 …
Modeling the formation and eruption of coronal structures by linking data-driven magnetofrictional and MHD simulations for AR 12673
Context. The data-driven and time-dependent modeling of coronal magnetic fields is crucial
for understanding solar eruptions. These efforts are complicated by the challenges of finding …
for understanding solar eruptions. These efforts are complicated by the challenges of finding …
Detection of the strongest magnetic field in a sunspot light bridge
Traditionally, the strongest magnetic fields on the Sun have been measured in sunspot
umbrae. More recently, however, much stronger fields have been measured at the ends of …
umbrae. More recently, however, much stronger fields have been measured at the ends of …
Data-driven, time-dependent modeling of pre-eruptive coronal magnetic field configuration at the periphery of NOAA AR 11726
E Lumme, J Pomoell, DJ Price, EKJ Kilpua… - Astronomy & …, 2022 - aanda.org
Context. Data-driven, time-dependent magnetofrictional modeling has proved to be an
efficient tool for studying the pre-eruptive build-up of energy for solar eruptions, and …
efficient tool for studying the pre-eruptive build-up of energy for solar eruptions, and …
A study of pre-flare solar coronal magnetic fields: magnetic flux ropes
Magnetic flux ropes (MFRs) are thought to be the central structures of solar eruptions, and
their ideal MHD instabilities can trigger the eruption. Here we performed a study of all the …
their ideal MHD instabilities can trigger the eruption. Here we performed a study of all the …
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 Xia… - 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 …