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20112026
most citedRecurrent Two-Sided Loop Jets Caused by Magnetic Reconnection between Erupting Minifilaments and Nearby Large Filament

36 citations · 184 across the 13 of their papers we have counts for

collaborators

15 papers

astro-ph.SR2026

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…

astro-ph.SR2026

HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager

Zou SiZhong, Liu Hui, Su Yang +5

Solar flare hard X-ray imaging is a key diagnostic of flare energy release and electron acceleration. The Hard X-ray Imager (HXI) aboard ASO-S compresses the two-dimensional source…

astro-ph.SR2026

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…

astro-ph.SR2025★ 3 cited

Resolving Interchange Reconnection Dynamics in a Fan-Spine-like Topology Observed by Solar Orbiter

Yadan Duan, Xiaoli Yan, Junchao Hong +5

Interchange reconnection is believed to play a significant role in the production of solar jets and solar wind. However, the dynamics of interchange reconnection in the low corona…

astro-ph.SR2025

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…

astro-ph.SR2025

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…

astro-ph.SR2024

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…

astro-ph.SR2024

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…

astro-ph.SR2023★ 8 cited

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…

astro-ph.SR2021★ 25 cited

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…

astro-ph.SR2021★ 23 cited

Direct Observation of A Large-scale CME Flux Rope Event Arising from an Unwinding Coronal Jet

Hechao Chen, Jiayan Yang, Junchao Hong +2

Coronal mass ejections (CMEs) and coronal jets are two types of common solar eruptive phenomena, which often independently happen at different spatial scales. In this work, we pres…

astro-ph.SR2019★ 36 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.SR2019★ 35 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.SR2018★ 20 cited

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…

astro-ph.SR2011★ 34 cited

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…