6 papers
From Photospheric Footpoint Motion to Plasmoid Ejection: A Two-Stage Reconnection Process in a Small-scale Chromospheric Jet
Zehao Tang, Yuandeng Shen, Chengrui Zhou +3
Using high spatiotemporal resolution, multi-wavelength observations from the New Vacuum Solar Telescope (NVST) and the Solar Dynamics Observatory (SDO), we present a detailed analy…
How Reconnection-Unfavored Magnetic Flux Emergence Suppresses Solar Filament Eruptions
Chengrui Zhou, Yuandeng Shen, Chun Xia +4
Magnetic flux emergence is traditionally considered a key trigger of solar filament eruptions; however, its role in suppressing filament eruptions remains less understood. Using mu…
Deciphering the Formation and Dynamics of Double-decker Filament Through Component Magnetic Reconnection
Dongxu Liu, Yuandeng Shen, Yi Bi +3
The formation of double-decker filaments has long been an enigma in the field of solar physics. Using stereoscopic observations from the Solar Dynamics Observatory and the Solar Te…
High-Resolution Observations of a Small-Scale Cancellation Nanoflare: Supporting Evidence for the Cancellation Nanoflare Model
Zehao Tang, Yuandeng Shen, Chengrui Zhou +2
An analytical cancellation nanoflare model has recently been established to show the fundamental role that ubiquitous small-scale cancellation nanoflares play in solar atmospheric…
A New Formation Mechanism of Counterstreaming Mass Flows in Filaments and the Doppler Bullseye Pattern in Prominences
Chengrui Zhou, Yuandeng Shen, Chun Xia +3
The eruption of solar prominences can eject substantial mass and magnetic field into interplanetary space and cause geomagnetic storms. However, various questions about prominences…
Formation and Eruption of Hot Channel Magnetic Flux Rope in Nested Double Null Magnetic System
Surui Yao, Yuandeng Shen, Chengrui Zhou +2
The coronal magnetic topology significantly affects the outcome of magnetic flux rope (MFR) eruptions. The recently reported nested double null magnetic system remains unclear as t…