Recurrent Jetlets Associated with the Disappearance of a Satellite Spot
Liheng Yang, Xiaoli Yan, Jun Zhang, Zhike Xue, Zhe Xu, Jincheng Wang, Yijun Hou, Yian Zhou, Defang Kong, Roslan Umar, Xinsheng Zhang, Qiaoling Li, Liping Yang

TL;DR
This study investigates recurrent jetlets from a satellite spot in the solar atmosphere, revealing their connection to magnetic cancellation, mini-flux-rope eruptions, and 3D magnetic reconnection, using high-resolution multi-wavelength data.
Contribution
It provides new insights into the physical mechanisms behind recurrent jetlets, linking them to magnetic flux cancellation and mini-flux-rope eruptions in the solar atmosphere.
Findings
Jetlets have widths of 1300-2900 km and last 3-10 minutes.
Satellite spot moved northwest at 376 m/s during eruptions.
Magnetic cancellation rate was 1.3×10^{18} Mx/hr, driving jetlets.
Abstract
Recurrent small-scale eruptions are fascinating phenomena in the solar atmosphere. However, their underlying physical mechanisms remain unclear. On 2021 May 23, five recurrent jetlets (J1-J5) were observed continuously ejecting from a satellite spot located at the north edge of AR 12824. Using high-resolution, multi-wavelength data from NVST, SDO, and IRIS, we investigate the physical characteristics of these jetlets and their relationship with the satellite spot. The widths of these jetlets range from 1300 to 2900 km, their lifetimes range span 3 to 10 minutes, and their projection speeds vary from 152.8 to 406.0 km s. During the eruptions, the satellite spot moved northwest at a low speed of 376 12 m s. Its area gradually decreased due to magnetic cancellation with surrounding positive magnetic field, resulting in an average cancellation rate of…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Astrophysics and Cosmic Phenomena · Astrophysical Phenomena and Observations
