Observations of a Series of Flares and Associated Jet-like Eruptions Driven by the Emergence of Twisted Magnetic Fields
Eun-Kyung Lim, Vasyl Yurchyshyn, Sung-Hong Park, Sujin Kim, Kyung-Suk, Cho, Pankaj Kumar, Jongchul Chae, Heesu Yang, Kyuhyoun Cho, Donguk Song, and, Yeon-Han Kim

TL;DR
This study observes a sequence of solar flares and jet-like eruptions driven by emerging twisted magnetic fields, revealing the evolution of jet structures and magnetic properties through high-resolution solar observations.
Contribution
It provides new insights into how emerging twisted magnetic flux influences the development of successive flares and blowout jets on the Sun.
Findings
Jets evolved from inverted-Y shapes to twisted structures.
Magnetic flux and helicity increased gradually before and during flares.
Continuous magnetic twist emergence is linked to flare and jet activity.
Abstract
We studied temporal changes of morphological and magnetic properties of a succession of four confined flares followed by an eruptive flare using the high-resolution New Solar Telescope (NST) operating at the Big Bear Solar Observatory (BBSO), Helioseismic and Magnetic Imager (HMI) magnetograms and Atmospheric Image Assembly (AIA) EUV images provided by Solar Dynamics Observatory (SDO). From the NST/Halpha and the SDO/AIA~304 A observations we found that each flare developed a jet structure that evolved in a manner similar to evolution of the blowout jet : 1) an inverted-Y shape jet appeared and drifted away from its initial position; 2) jets formed a curtain-like structure that consisted of many fine threads accompanied with subsequent brightenings near the footpoints of the fine threads; and finally 3) the jet showed a twisted structure visible near the flare maximum. Analysis of the…
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