19 citations · 35 across the 6 of their papers we have counts for
6 papers
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…
Data-constrained 3D MHD Simulation of a Spiral Jet Caused by an Unstable Flux Rope Embedded in Fan-spine Configuration
Z. F. Li, J. H. Guo, X. Cheng +5
Spiral jets are impulsive plasma ejections that typically show an apparent rotation motion. Their generation, however, is still nont understood thoroughly. Based on a high-resoluti…
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…
Filament eruption by multiple reconnections
Y. Liu, G. P. Ruan, B. Schmieder +5
Filament eruption is a common phenomenon in solar activity, but the triggering mechanism is not well understood. We focus our study on a filament eruption located in a complex nest…
Decayless longitudinal oscillations of a solar filament maintained by quasi-periodic jets
Y. W. Ni, J. H. Guo, Q. M. Zhang +3
Context: As a ubiquitous phenomenon, large-amplitude longitudinal filament oscillations usually decay in 1--4 periods. Recently, we observed a decayless case of such oscillations i…
Grow-up of a Filament Channel by Intermittent Small-scale Magnetic Reconnection
H. T. Li, X. Cheng, J. H. Guo +5
Filament channel (FC), a plasma volume where the magnetic field is primarily aligned with the polarity inversion line, is believed to be the pre-eruptive configuration of coronal m…