A Possible Mechanism for the “Late Phase” in Stellar White-light Flares

KE Yang, X Sun, GS Kerr… - The Astrophysical …, 2023 - iopscience.iop.org
M dwarf flares observed by the Transiting Exoplanet Survey Satellite (TESS) sometimes
exhibit a peak-bump light-curve morphology, characterized by a secondary, gradual peak …

From fundamental theory to realistic modeling of the birth of solar eruptions

C Jiang - Science China Earth Sciences, 2024 - Springer
Solar eruptions, primarily manifested as solar flares, filament eruptions and coronal mass
ejections, represent explosive releases of magnetic energy stored in the solar corona, with …

Modeling the propagation of coronal mass ejections with COCONUT: Implementation of the regularized Biot-Savart law flux rope model

JH Guo, L Linan, S Poedts, Y Guo, A Lani… - Astronomy & …, 2024 - aanda.org
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 …

Magnetic flux rope models and data-driven magnetohydrodynamic simulations of solar eruptions

Y Guo, J Guo, Y Ni, C **a, Z Zhong, M Ding… - Reviews of Modern …, 2024 - Springer
Solar eruptive activities, such as flares, coronal mass ejections (CMEs), and prominence or
filament eruptions, pose both scientific and practical challenges to human beings. To …

[HTML][HTML] From kink instability to magnetic reconnection to oscillations in solar flares

PK Browning, M Gordovskyy, LACA Schiavo… - Fundamental Plasma …, 2024 - Elsevier
We show how some different fundamental plasma processes-the ideal kink instability,
magnetic reconnection and magnetohydrodynamic oscillations-can be causally linked. This …

[PDF][PDF] Fundamental Plasma Physics

PK Browning, M Gordovskyy, LACA Schiavo, J Stewart - researchgate.net
We show how some different fundamental plasma processes-the ideal kink instability,
magnetic reconnection and magnetohydrodynamic oscillations-can be causally linked. This …