Stereoscopic Observations of an Erupting Mini-filament-driven Two-sided-loop Jet and the Applications for Diagnosing a Filament Magnetic Field

• Published in: The Astrophysical journal Vol. 883; no. 1; pp. 104 - 113
• Main Authors: Shen, Yuandeng, Qu, Zhining, Yuan, Ding, Chen, Huadong, Duan, Yadan, Zhou, Chengrui, Tang, Zehao, Huang, Jin, Liu, Yu
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 20-09-2019; IOP Publishing
• Subjects: Astrophysics; Magnetic fields; Magnetic structure; Observatories; Solar activity; Solar atmosphere; Solar coronal mass ejections; Solar filaments; Solar flares; Solar magnetic field; Solar magnetic fields; Solar wind; Stereoscopy
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/ab3a4d

Ubiquitous solar jets or jet-like activities are generally regarded as an important source of energy and mass input to the upper solar atmosphere and the solar wind. However, their triggering and driving mechanisms are not completely understood. By taking advantage of stereoscopic observations with high temporal and spatial resolutions taken by the Solar Dynamic Observatory (SDO) and the Solar Terrestrial Relations Observatory (STEREO), we report an intriguing two-sided-loop jet that occurred on 2013 June 02, and was dynamically associated with the eruption of a mini-filament below an overlying large filament. Additionally, two distinct reconnection processes are identified during the formation stage. The SDO observations reveal that the two-sided-loop jet showed a concave shape with a projection speed of about 80-136 km s−1. From the other view angle, the STEREO observations clearly showed that the trajectories of the two arms of the two-sided-loop were along the cavity magnetic field lines hosting the large filament. Contrary to the well-accepted theoretical model, the present observation sheds new light on our understanding of the formation mechanism of two-sided-loop jets. Moreover, the eruption of the two-sided-loop jet not only supplied mass to the overlying large filament, but also provided a rare opportunity to diagnose the magnetic structure of the overlying large filament via the method of three-dimensional reconstruction.