activity
20152020
most citedPartial eruption of a filament with twisting nonuniform fields

44 citations · 138 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2020

Dynamics of descending knots in a solar prominence and their possible contributions to the heating of the local corona

Yi Bi, Bo Yang, Tng Li +2

The knots in solar prominences are often observed to fall with nearly constant velocity, but the associated physical mechanism is currently not well understood. In this letter, we…

astro-ph.SR201936 cited

Recurrent Two-Sided Loop Jets Caused by Magnetic Reconnection between Erupting Minifilaments and Nearby Large Filament

Bo Yang, Jiayan Yang, Yi Bi +4

Using high spatial and temporal data from the New Vacuum Solar Telescope (NVST) and the Solar Dynamics Observatory (SDO), we present unambiguous observations of recurrent two-sided…

astro-ph.SR201912 cited

Two-step evolution of a rising flux rope resulting in a confined solar flare

Shuhong Yang, Jun Zhang, Qiao Song +2

Combining the Solar Dynamics Observatory and the New Vacuum Solar Telescope observations, we study a confined flare triggered by a rising flux rope within the trailing sunspots of…

astro-ph.SR201935 cited

Observation of a reversal of breakout reconnection preceding a jet: evidence of oscillatory magnetic reconnection?

Junchao Hong, Jiayan Yang, Huadong Chen +3

Recent studies have revealed that solar jets involving minifilament eruptions may be initiated under the well-known magnetic-breakout mechanism. Before or just at the onset of thos…

astro-ph.SR201811 cited

Untwisting and Disintegration of a Solar Filament Associated with Photospheric Flux Cancellation

Huadong Chen, Ruisheng Zheng, Leping Li +3

Using the high-resolution observations from New Vacuum Solar Telescope (NVST) jointly with the Solar Dynamics Observatory data, we investigate two successive confined eruptions (Er…

astro-ph.SR2018

A Survey of Changes in Magnetic Helicity Flux on the Photosphere During Relatively Low Class Flares

Yi Bi, Ying D Liu, Yanxiao Liu +3

Using the 135-second cadence of the photospheric vector data provided by the Helioseismic and Magnetic Imager telescope on board the Solar Dynamic Observatory, we examined the time…