This paper explores the evolution of geoscientific inquiry, tracing the progression from
traditional physics-based models to modern data-driven approaches facilitated by significant …

Solar eruptions are outbursts of magnetized plasma in the atmosphere of the Sun,
encompassing phenomena like solar flares, ejective prominences and coronal mass …

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 …

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 …

Solar filaments often exhibit rotation and deflection during eruptions, which would
significantly affect the geoeffectiveness of the corresponding coronal mass ejections …

There is a heated debate regarding the specific roles played by ideal magnetohydrodynamic
(MHD) instability and magnetic reconnection in triggering solar eruptions. In the context of a …

We present a method of conducting data-driven simulations of solar active regions and flux
emergence with the MURaM radiative magnetohydrodynamics (MHD) code. The horizontal …

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 …

We analyze the forces that control the dynamic evolution of a flux rope eruption in a three-
dimensional radiative magnetohydrodynamic simulation. The confined eruption of the flux …

Two major mechanisms have been proposed to drive the solar eruptions: the ideal
magnetohydrodynamic instability and the resistive magnetic reconnection. Due to the close …