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20212026
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 · 47 across the 18 of their papers we have counts for

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Showing 2023Show all

7 papers · 1 filter

astro-ph.SR2023

Rotation and Confined Eruption of a Double Flux-Rope System

Xiaomeng Zhang, Jinhan Guo, Yang Guo +2

We perform a data-constrained simulation with the zero- assumption to study the mechanisms of strong rotation and failed eruption of a filament in active region 11474 on 2012 Ma…

astro-ph.SR2023

Observational study of intermittent solar jets: p-mode modulation

Qiuzhuo Cai, Guiping Ruan, Chenxi Zheng +7

Aims. Recurring jets are observed in the solar atmosphere, which can erupt intermittently. By the observation of intermittent jets, we want to understand the causes of periodic eru…

astro-ph.SR2023★ 6 cited

A Method for Determining the Locations and Configurations of Magnetic Reconnection within 3D Turbulent Plasmas

Yulei Wang, Xin Cheng, Yang Guo +2

Context. Three-dimensional (3D) reconnection is an important mechanism for efficiently releasing energy during astrophysical eruptive events, which is difficult to be quantitativel…

astro-ph.SR2023★ 1 cited

Modelling the propagation of coronal mass ejections with COCONUT: implementation of the Regularized Biot-Savart Laws flux rope model

Jinhan Guo, L. Linan, S. Poedts +8

Context: Coronal mass ejections (CMEs) are rapid eruptions of magnetized plasma that occur on the Sun, which are known as the main drivers of adverse space weather. Accurately trac…

astro-ph.SR2023

Data-constrained Magnetohydrodynamic Simulation of an Intermediate Solar Filament Eruption

Yang Guo, Jinhan Guo, Yiwei Ni +5

Solar eruptive activities could occur in weak magnetic field environments and over large spatial scales, especially relevant to eruptions involving intermediate or quiescent solar…

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.SR2023★ 39 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…