Publications (11)
Two-sided-loop jet originates from the filament internal reconnection
Yunxue Huang, Jialin Li, Zhining Qu +4
Magnetic reconnection driving two-sided-loop jet is typically associated with interactions between an emerging bipole and the overlying horizontal magnetic field, or between filame…
On a solar blowout jet: driven mechanism and the formation of cool and hot components
Yuandeng Shen, Ying D. Liu, Jiangtao Su +2
We present the observations of a blowout jet that experienced two distinct ejection stages. The first stage started from the emergence of a small positive magnetic polarity, which…
Round-trip Slipping Motion of the Circular Flare Ribbon Evidenced in a Fan-spine Jet
Yuandeng Shen, Zhining Qu, Chengrui Zhou +3
A solar jet on 2014 July 31, which was accompanied by a GOES C1.3 flare and a mini-filament eruption at the jet base, was studied by using observations taken by the New Vacuum Sola…
Broad and Bi-directional narrow quasi-periodic fast-propagating wave trains associated with a filament-driven halo CME on 2023 April 21
Xinping Zhou, Yuandeng Shen, Yihua Yan +8
This paper presents three distinct wave trains that occurred on 2023 April 21: a broad quasi-periodic fast-propagating (QFP) wave train and a bi-directional narrow QFP wave train.…
On the origin of a broad QFP wave train: unwinding jet as the driver
Xinping Zhou, Zehao Tang, Zhining Qu +5
Large-scale extreme-ultraviolet (EUV) waves commonly exhibit as single wavefront and are believed to be caused by coronal mass ejections (CMEs). Utilizing high spatiotemporal resol…
Double-decker Pair of Flux Ropes Formed by Two Successive Tether-cutting Eruptions
Yuandeng Shen, Dongxu Liu, Surui Yao +7
Double-decker filaments and their eruptions have been widely observed in recent years, but their physical formation mechanism is still unclear. Using high spatiotemporal resolution…
White-light QFP Wave Train and the Associated Failed Breakout Eruption
Yuandeng Shen, Surui Yao, Zehao Tang +5
Quasi-periodic fast-propagating (QFP) magnetosonic wave trains are commonly observed in the low corona at extreme ultraviolet wavelength bands. Here, we report the first white-ligh…
Stereoscopic Observations of an Erupting Mini-filament Driven Two-Sided-Loop Jet and the Applications for Diagnosing Filament Magnetic field
Yuandeng Shen, Zhining Qu, Ding Yuan +6
The ubiquitous solar jets or jet-like activities are generally regarded as an important source of energy and mass input to the upper solar atmosphere and the solar wind. However, q…
On a small-scale EUV wave: the driving mechanism and the associated oscillating filament
Yuandeng Shen, Yu Liu, Zhanjun Tian +1
We present observations of a small-scale Extreme-ultraviolet (EUV) wave that was associated with a mini-filament eruption and a GOES B1.9 micro-fare in the quiet Sun region. The in…
Recurrent narrow quasi-periodic fast-propagating wave trains excited by the intermittent energy release in the accompanying solar flare
Xinping Zhou, Yuandeng Shen, Hongfei Liang +5
About the driven mechanisms of the quasi-periodic fast-propagating (QFP) wave trains, there exist two dominant competing physical explanations: associated with the flaring energy r…
3D fast-mode Wave Propagation from Corona to Chromosphere: Triggering Mechanism for 3D Oscillations of filaments
Yunxue Huang, Qin Feng, Yuhu Miao +5
Moreton waves are widely regarded as the chromospheric counterpart of extreme ultraviolet (EUV) waves propagating in the corona. However, direct observational evidence confirming t…