Extreme solar events
EW Cliver, CJ Schrijver, K Shibata… - Living Reviews in Solar …, 2022 - Springer
We trace the evolution of research on extreme solar and solar-terrestrial events from the
1859 Carrington event to the rapid development of the last twenty years. Our focus is on the …
1859 Carrington event to the rapid development of the last twenty years. Our focus is on the …
Magnetic reconnection: MHD theory and modelling
In this review we focus on the fundamental theory of magnetohydrodynamic reconnection,
together with applications to understanding a wide range of dynamic processes in the solar …
together with applications to understanding a wide range of dynamic processes in the solar …
Broadening and redward asymmetry of Hα line profiles observed by LAMOST during a stellar flare on an M-type star
Stellar flares are characterized by sudden enhancement of electromagnetic radiation in
stellar atmospheres. So far, much of our understanding of stellar flares has come from …
stellar atmospheres. So far, much of our understanding of stellar flares has come from …
Observation of two splitting processes in a partial filament eruption on the sun: the role of breakout reconnection
Partial filament eruptions have often been observed; however, the physical mechanisms that
lead to filament splitting are not yet fully understood. In this study, we present a unique event …
lead to filament splitting are not yet fully understood. In this study, we present a unique event …
Possible detection of coronal mass ejections on late-type main-sequence stars in LAMOST medium-resolution spectra
Context. Stellar coronal mass ejections (CMEs) are the primary driver of exoplanetary space
weather and may affect the habitability of exoplanets. However, detections of possible stellar …
weather and may affect the habitability of exoplanets. However, detections of possible stellar …
Toward improved understanding of magnetic fields participating in solar flares: Statistical analysis of magnetic fields within flare ribbons
MD Kazachenko, BJ Lynch, A Savcheva… - The Astrophysical …, 2022 - iopscience.iop.org
Violent solar flares and coronal mass ejections (CMEs) are magnetic phenomena. However,
how magnetic fields reconnecting in the flare differ from nonflaring magnetic fields remains …
how magnetic fields reconnecting in the flare differ from nonflaring magnetic fields remains …
A Study of Preflare Solar Coronal Magnetic Fields: Magnetic Energy and Helicity
Solar flares fall into two types, with eruptive ones associated with coronal mass ejection
(CME) and confined ones without CME. To explore whether there are preflare conditions in …
(CME) and confined ones without CME. To explore whether there are preflare conditions in …
Survey of Magnetic Field Parameters Associated with Large Solar Flares
T Li, Y Zheng, X Li, Y Hou, X Li, Y Zhang… - The Astrophysical …, 2024 - iopscience.iop.org
Until now, how the magnetic fields in M/X-class flaring active regions (ARs) differ from C-
class flaring ARs remains unclear. Here, we calculate the key magnetic field parameters …
class flaring ARs remains unclear. Here, we calculate the key magnetic field parameters …
[HTML][HTML] Stellar Flares, Superflares, and Coronal Mass Ejections—Entering the Big Data Era
K Vida, Z Kővári, M Leitzinger, P Odert, K Oláh, B Seli… - Universe, 2024 - mdpi.com
Flares, sometimes accompanied by coronal mass ejections (CMEs), are the result of sudden
changes in the magnetic field of stars with high energy release through magnetic …
changes in the magnetic field of stars with high energy release through magnetic …
Multiwavelength signatures of episodic nullpoint reconnection in a quadrupolar magnetic configuration and the cause of failed flux rope eruption
In this paper, we present multiwavelength observations of the triggering of a failed-eruptive
M-class flare from active region NOAA 11302 and investigate the possible reasons for the …
M-class flare from active region NOAA 11302 and investigate the possible reasons for the …