An EUV jet driven by a series of transition region micro-jets Article Swipe

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Hengyuan Wei , Zhenghua Huang , Hui Fu , Ming Xiong , Lidong Xia , Chao Zhang , Kaiwen Deng , Haiyi Li ·

YOU? · · 2022 · Open Access · · DOI: https://doi.org/10.48550/arxiv.2208.00112

Jets are one of the most common eruptive events in the solar atmosphere, and they are believed to be important in the context of coronal heating and solar wind acceleration. We present an observational study on a sequence of jets with the data acquired with the Solar Dynamics Observatory (SDO) and the Interface Region Imaging Spectrograph (IRIS). This sequence is peculiar in that an EUV jet, $\sim29\arcsec$ long and with a dome-like base, appears to be a consequence of a series of transition region (TR) micro-jets that are a few arcsecs in length.We find that the occurrence of any TR micro-jets is always associated with the change of geometry of micro-loops at the footpoints of the microjets. A bundle of TR flux ropes is seen to link a TR micro-jet to the dome-like structure at the base of the EUV jet. This bundle rises as a response to the TR micro-jets, with the rising motion eventually triggering the EUV jet. We propose a scenario involving a set of magnetic reconnections, in which the series of TR micro-jets are associated with the processes to remove the constraints to the TR flux ropes and thus allow them to rise and trigger the EUV jet. Our study demonstrates that small-scale dynamics in the lower solar atmosphere are crucial in understanding the energy and mass connection between the corona and the solar lower atmosphere, even though many of them might not pump mass and energy to the corona directly.

Related Topics

Physics

Astrophysics

Extreme Ultraviolet Lithography

Coronal Mass Ejection

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Physics Jet (fluid) Astrophysics Extreme ultraviolet lithography Coronal mass ejection Corona (planetary geology) Atmosphere (unit) Context (archaeology) Solar observatory Magnetic reconnection Coronal hole Astronomy Plasma Solar wind Mechanics Optics Meteorology Magnetic field Nuclear physics Biology Paleontology Venus Astrobiology Quantum mechanics

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Type: preprint
Language: en
Landing Page: http://arxiv.org/abs/2208.00112
PDF: https://arxiv.org/pdf/2208.00112
OA Status: green
Related Works: 10
OpenAlex ID: https://openalex.org/W4289645250

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DOI: https://doi.org/10.48550/arxiv.2208.00112

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Title: An EUV jet driven by a series of transition region micro-jets

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Type: preprint

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Language: en

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Publication year: 2022

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Publication date: 2022-07-30

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Authors: Hengyuan Wei, Zhenghua Huang, Hui Fu, Ming Xiong, Lidong Xia, Chao Zhang, Kaiwen Deng, Haiyi Li

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Landing page: https://arxiv.org/abs/2208.00112

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Concepts: Physics, Jet (fluid), Astrophysics, Extreme ultraviolet lithography, Coronal mass ejection, Corona (planetary geology), Atmosphere (unit), Context (archaeology), Solar observatory, Magnetic reconnection, Coronal hole, Astronomy, Plasma, Solar wind, Mechanics, Optics, Meteorology, Magnetic field, Nuclear physics, Biology, Paleontology, Venus, Astrobiology, Quantum mechanics

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