Two-sided-loop Jet Originates from the Filament Internal Reconnection

Abstract Magnetic reconnection driving a two-sided-loop jet is typically associated with interactions between an emerging bipole and the overlying horizontal magnetic field, or between filaments from separate magnetic systems. Leveraging high temporal and spatial resolution observations from ground-based and space-borne instruments, we have identified a two-sided-loop jet originating from magnetic reconnection between threads within a single filament. Our observations show that as two initially crossing filamentary threads within the filament converge, reconnection takes place at their intersection. In the Doppler images, distinct redshift and blueshift signals are observed at the locations where the filament threads intersected. This process generates a two-sided-loop jet with outflow speeds of 22.2 and 62.5 km s −1 . Following reconnection, the original crossing threads transform into two parallel threads that subsequently separate at speeds of 2.8 and 8.3 km s −1 . This observation offers a new perspective on the mechanisms responsible for jet formation.

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Publication Details

Journal
Research in Astronomy and Astrophysics
Published
2025-08-28
DOI
https://doi.org/10.1088/1674-4527/ae0079
Citations
1
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
1.15
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article

Two-sided-loop Jet Originates from the Filament Internal Reconnection

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1 citations
Research in Astronomy and Astrophysics
Solar and Space Plasma Dynamics
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article

Two-sided-loop Jet Originates from the Filament Internal Reconnection

Ke Yu, Rui Xue, Zhisong Qu, Xinping Zhou, Hongfei Liang, Jialin Li, Y. J. Huang
article en
1 citations

Abstract

Abstract Magnetic reconnection driving a two-sided-loop jet is typically associated with interactions between an emerging bipole and the overlying horizontal magnetic field, or between filaments from separate magnetic systems. Leveraging high temporal and spatial resolution observations from ground-based and space-borne instruments, we have identified a two-sided-loop jet originating from magnetic reconnection between threads within a single filament. Our observations show that as two initially crossing filamentary threads within the filament converge, reconnection takes place at their intersection. In the Doppler images, distinct redshift and blueshift signals are observed at the locations where the filament threads intersected. This process generates a two-sided-loop jet with outflow speeds of 22.2 and 62.5 km s −1 . Following reconnection, the original crossing threads transform into two parallel threads that subsequently separate at speeds of 2.8 and 8.3 km s −1 . This observation offers a new perspective on the mechanisms responsible for jet formation.

Research in Astronomy and AstrophysicsVol. 25(11)
Yunnan Normal University (CN), Zhejiang Normal University (CN), Sichuan Normal University (CN)
Openalex Percentile: Top 17%
Solar and Space Plasma Dynamics
1.15
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