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Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops
Leping Li, Hongqiang Song, Yijun Hou +11
Failure of a filament eruption caused by magnetic reconnection between the erupting filament and the overlying magnetic field has been previously proposed in numerical simulations.…
Alpha-Proton Differential Flow of A Coronal Mass Ejection at 15 Solar Radii
Xuechao Zhang, Hongqiang Song, Xiaoqian Wang +4
Alpha-proton differential flow () of coronal mass ejections (CMEs) and solar wind from the Sun to 1 au and beyond could influence the instantaneous correspondence of absol…
Comparison of Ion-Proton Differential Speed between ICMEs and Solar Wind near 1 au
Xuechao Zhang, Hongqiang Song, Chengxiao Zhang +6
The elemental abundance of ICMEs and solar wind near 1 au is often adopted to represent the abundance in the corresponding coronal sources. However, the absolute abundance of heavy…
Eruption of a million-Kelvin warm magnetic flux rope on the Sun
Leping Li, Hongqiang Song, Hardi Peter +4
Solar magnetic flux rope (MFR) plays a central role in the physics of coronal mass ejections (CMEs). It mainly includes a cold filament at typical chromospheric temperatures (10000…