207 citations · 2.4k across the 65 of their papers we have counts for
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Total reflection of a flare-driven quasi-periodic EUV wave train at a coronal hole boundary
Xinping Zhou, Yuandeng Shen, Zehao Tang +3
The reflection, refraction, and transmission of large-scale extreme ultraviolet (EUV) waves (collectively, secondary waves) have been observed during their interactions with corona…
Coronal Quasi-periodic Fast-mode Propagating Wave Trains
Yuandeng Shen, Xinping Zhou, Yadan Duan +3
QFP wave trains in the corona have been studied intensively in the past decade, thanks to the full-disk, high spatiotemporal resolution, and wide-temperature coverage observations…
Sympathetic Filament Eruptions within a Fan-spine Magnetic System
Chengrui Zhou, Yuandeng Shen, Xinping Zhou +3
It is unclear whether successive filament eruptions at different sites within a short time interval are physically connected or not. Here, we present the observations of the succes…
CME-Driven and Flare-Ignited Fast Magnetosonic Waves Successively Detected in a Solar Eruption
Xinping Zhou, Yuandeng Shen, Jiangtao Su +4
We present SDO/AIA observation of three types of fast-mode propagating magnetosonic waves in a GOES C3.0 flare on 2013 April 23, which was accompanied by a prominence eruption and…
Sympathetic Standard and Blowout Coronal Jets Observed in a Polar Coronal Hole
Zehao Tang, Yuandeng Shen, Xinping Zhou +4
We present the sympathetic eruption of a standard and a blowout coronal jets originating from two adjacent coronal bright points (CBP1 and CBP2) in a polar coronal hole, using soft…
Measuring three-dimensional shapes of stable solar prominences using stereoscopic observations from SDO and STEREO
Chengrui Zhou, Chun Xia, Yuandeng Shen
Although the real shapes and trajectories of erupting solar prominences in three dimensions have been intensively studied, the three-dimensional (3D) shapes of stable prominences b…
Observation and Modeling of Solar Jets
Yuandeng Shen
The solar atmosphere is full of complicated transients manifesting the reconfiguration of solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma ejectio…