The Action of the Collisional Shearing Mechanism in Complex Emerging and Developing Active Regions Revealed by SDO and Hinode Observations and Data-Driven Modeling
Abstract
Active Regions (ARs) in their emergence phase are known to be more flare productive and eruptive than ARs in their decay phase. In this work, we focus on complex emerging ARs composed of multiple bipoles. Due to the compact clustering of the different emerging bipoles within such complex multipolar ARs, collision and shearing between opposite non-conjugated polarities produces "collisional polarity inversion lines" (cPILs) and drives rapid photospheric cancellation of magnetic flux. The strength and the duration of the collision, shearing, and cancellation is defined by the natural separation of the conjugated polarities during the emergence phase of each bipole in the AR. This mechanism is called "collisional shearing". In Chintzoglou et al (2019), it was demonstrated that collisional shearing occurred in two emerging flare- and CME-productive ARs (NOAA AR11158 and AR12017) by measuring significant amounts of magnetic flux cancelling at the cPIL. This finding supported the formation and energization of magnetic flux ropes before their eruption as CMEs and the associated flare activity. Here, we provide additional evidence from HINODE observations that confirm the occurrence of strong magnetic cancellation at the cPIL of these ARs. In addition, we provide results from data-driven 3D modeling of the coronal magnetic field, capturing the formation and evolution of the energized structures during the collisional shearing process. We discuss our results in relation to flare and eruptive activity.
- Publication:
-
43rd COSPAR Scientific Assembly. Held 28 January - 4 February
- Pub Date:
- January 2021
- Bibcode:
- 2021cosp...43E.991C