most citedThermodynamic and Magnetic Topology Evolution of the X1.0 Flare on 2021 October 28 Simulated by a Data-driven Radiative Magnetohydrodynamic Model

39 citations · 40 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2024

Periodic Coronal Rain Driven by Self-consistent Heating Process in a Radiative Magnetohydrodynamic Simulation

Zekun Lu, Feng Chen, J. H. Guo +5

The periodic coronal rain and in-phase radiative intensity pulsations have been observed in multiple wavelengths in recent years. However, due to the lack of three-dimensional coro…

astro-ph.SR2024

Recent advances in solar data-driven MHD simulations of the formation and evolution of CME flux ropes

Brigitte Schmieder, Jinhan Guo, Stefaan Poedts

Filament eruptions and coronal mass ejections are physical phenomena related to magnetic flux ropes carrying electric current. A magnetic flux rope is a key structure for solar eru…

astro-ph.SR20241 cited

How coronal mass ejections are influenced by the morphology and toroidal flux of their source magnetic flux ropes?

J. H. Guo, L. Linan, S. Poedts +9

Coronal mass ejections (CMEs) stand as intense eruptions of magnetized plasma from the Sun, playing a pivotal role in driving significant changes of the heliospheric environment. D…

astro-ph.SR2023

Data-driven Modeling of a Coronal Magnetic Flux Rope: from Birth to Death

J. H. Guo, Y. W. Ni, Y. Guo +7

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 geom…

astro-ph.SR2023

Understanding the Lateral Drifting of an Erupting Filament with a Data-constrained Magnetohydrodynamic Simulation

Jinhan Guo, Ye Qiu, Yiwei Ni +6

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

astro-ph.SR202339 cited

Thermodynamic and Magnetic Topology Evolution of the X1.0 Flare on 2021 October 28 Simulated by a Data-driven Radiative Magnetohydrodynamic Model

Jin-han Guo, Yi-wei Ni, Ze Zhong +6

Solar filament eruptions, flares and coronal mass ejections (CMEs) are manifestations of drastic release of energy in the magnetic field, which are related to many eruptive phenome…