6 papers
Data-driven Magnetohydrodynamic Simulation of the Initiation of a Coronal Mass Ejection with Multiple Stages
J. H. Guo, S. Poedts, B. Schmieder +8
Coronal mass ejections (CMEs) are the primary drivers of adverse space-weather events, yet their initiation and onset prediction remain insufficiently understood due to the complex…
Active region upflows in various coronal structures and their coupling to the lower atmosphere
Yingjie Zhu, Louise Harra, Krzysztof Barczynski +13
Plasma upflows with a Doppler shift exceeding -10 km/s at active region (AR) boundaries are considered potential sources of the nascent slow solar wind. We investigate the driving…
A unified model of solar prominence formation with self-consistent heating
C. J. Huang, Y. W. Ni, J. H. Guo +1
Several models have been proposed to explain the formation of solar prominences, among which the evaporation--condensation model and the direct injection model are the most popular…
Dependence of the intensity of the nonwave component of EUV waves on coronal magnetic field configuration
Yuwei Li, J. H. Guo, Y. W. Ni +2
Context. Mounting evidence has shown that EUV waves consist of a fast-mode magnetohydrodynamic (MHD) wave (or shock wave) followed by a slower nonwave component, as predicted by th…
Acceleration noise due to Space Magnetic Field for Heliocentric Gravitational Wave Detector
Peng Jia-Hui, Zhang Ji-Xiang, Hong W +4
The space-borne gravitational wave observatory is to detect low-frequency gravitational wave signals in the range of 0.1 mHz to 100 mHz. The inertial sensors of space gravitational…
The magnetic origin of the mystery of rare H Moreton waves
Ze Zhong, Yao Chen, Y. W. Ni +4
Over the past three decades, a lot of coronal fast-mode waves were detected by space missions, but their counterparts in the chromosphere, called the Moreton waves, were rarely cap…