Evolutionary stages and triggering process of a complex eruptive flare with circular and parallel ribbons
Navin Chandra Joshi (USO/PRL, Dept. of Phys./SRM Univ.), Bhuwan Joshi, (USO/PRL), Prabir K. Mitra (USO/PRL, Dept. of Phys./Gujarat Univ.)

TL;DR
This study analyzes a complex solar eruptive flare involving multiple ribbon types, revealing the magnetic topology and reconnection processes that trigger the eruption, highlighting the roles of null-point reconnection, flux rope dynamics, and instabilities.
Contribution
It provides a detailed multi-wavelength analysis of a complex flare with circular and parallel ribbons, emphasizing the magnetic topology and reconnection mechanisms involved.
Findings
Null-point reconnection initiates the flare.
Flux rope eruption triggers standard flare reconnection.
Both torus instability and breakout model contribute to eruption.
Abstract
We report multi-wavelength study of a complex M-class solar eruptive flare that consists of three different sets of flare ribbons, viz. circular, parallel, and remote ribbons. Magnetic field modeling of source active region NOAA 12242 exhibits the presence of 3D null-point magnetic topology which encompasses an inner bipolar region. The event initiates with the faint signatures of the circular ribbon along with remote brightening right from the pre-flare phase which points toward the ongoing slow yet persistent null-point reconnection. We first detected flux cancellation and an associated brightening, which are likely signatures of tether-cutting reconnection that builds the flux rope near the polarity inversion line (PIL) of the inner bipolar region. In the next stage, with the onset of M8.7 flare, there is a substantial enhancement in the brightening of circular ribbon which…
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