44 citations · 285 across the 20 of their papers we have counts for
22 papers
Sequential Magnetic Reconnections in a Fishbone-like Structure Leading to Recurrent Brightenings
Bo Yang, Jiayan Yang, Junchao Hong +1
The fine-scale release of magnetic free energy in the solar atmosphere is a fundamental open question in solar physics. Multi-wavelength observations at high spatiotemporal resolut…
Observational Evidence for Counter-helicity Magnetic Reconnection in a Solar Eruption
Jinrui Chang, Yi Bi, Bo Yang +3
Magnetic reconnection between coronal magnetic systems carrying opposite self-helicity may play a role in solar eruptions, but observational evidence remains limited. We investigat…
Machine Learning-based Separation of the He I 10830Å Chromospheric Signal: Quantitative Analysis of Chromosphere-Corona Intensity in the Quiet Sun
Huaiming Li, Fangyu Xu, Yi Bi +1
The He I 10830Å line, a crucial optically thin chromospheric line, is frequently used to study coronal heating and vertical coupling across the chromosphere-corona interface. Howev…
Sympathetic Eruption of Two Filaments and Associated Solar Coronal Jet
Jiayan Yang, Leping Li, Huadong Chen +4
Combining the high-quality observations from the {\it Solar Dynamics Observatory} (SDO), the Global Oscillation Network Group (GONG), and the Chinese H Solar Explorer (CHASE), w…
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…
Oscillatory magnetic reconnection at a coronal bright point
Junchao Hong, Jiayan Yang, Yi Bi +1
Coronal bright points are typical small-scale coronal brightenings that consist of a bundle of miniature coronal loops. Using the ultra-high-resolution coronal images from the Extr…
Moving Plasma Structures and Possible Driving Mechanisms of Solar Microflares Observed with High-Resolution Coronal Imaging
Qingmei Wang, Yi Bi, Hongfei Liang +2
Solar microflares are ubiquitous in the solar corona, yet their driving mechanisms remain a subject of ongoing debate. Using high-resolution coronal observations from the Solar Orb…
Observations of the Formation and Disappearance of a Funnel Prominence
Bo Yang, Jiayan Yang, Yi Bi +1
We present an observational study of the formation and disappearance of a funnel prominence. Before the funnel prominence formed, cool materials from the top of a preexisting polar…
Two-sided Loop Solar Jet Driven by the Eruption of a Small Filament in a Big Filament Channel
Jiayan Yang, Hechao Chen, Junchao Hong +2
Similar to the cases of anemone jets, two-sided loop solar jets could also be produced by either flux emergence from the solar interior or small scale filament eruptions. Using the…
Morphological evidence for nanoflares heating warm loops in the solar corona
Y. Bi, J. J. Yang, Y. Qin +6
Nanoflares are impulsive energy releases by magnetic reconnection in the braided coronal magnetic field, which is a potential mechanism for heating the corona. However, there are s…
Formation of a Solar Filament by Magnetic Reconnection and Associated Chromospheric Evaporation and Subsequent Coronal Condensation
Bo Yang, Jiayan Yang, Yi Bi +2
We present the first observation of a solar filament formed by magnetic reconnection and associated chromospheric evaporation and subsequent coronal condensation. Driven by shearin…
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…
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…
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…
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…
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…
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…
Observational Evidence of Magnetic Reconnection Associated with Magnetic Flux Cancellation
Bo Yang, Jiayan Yang, Yi Bi +4
Using high spatial and temporal data from the \emph{Solar Dynamics Observatory} (\emph{SDO}) and the \emph{Interface Region Imaging Spectrograph} (\emph{IRIS}), several observation…
The Formation of a Small-scale Filament after Flux Emergence on the Quiet Sun
Hechao Chen, Jiayan Yang, Bo Yang +2
We present observations of the formation process of a small-scale filament on the quiet Sun during 5-6 February 2016 and investigate its formation cause. Initially, a small dipole…
Partial eruption of a filament with twisting nonuniform fields
Yi Bi, Yunchun Jiang, Jiayan Yang +3
The eruption of the filament with the kink fashion is often regarded as a signature of the kink instability. However, the kink instability threshold for the filament magnetic struc…
The surge-like eruption of a miniature filament
Jia-Yan Yang, Yun-Chun Jiang, Dan Yang +4
We report on the rare eruption of a miniature H_alpha filament that took a surge form. The filament first underwent a full development within 46 minutes and then began to erupt 9 m…
Observations of EUV and Soft X-ray Recurring Jets in an Active Region
Liheng Yang, Yunchun Jiang, Jiayan Yang +3
We present simultaneous observations of three recurring jets in EUV and soft X-ray (SXR), which occurred in an active region on 2007 June 5. By comparing their morphological and ki…