Initiation and Eruption Process of Magnetic Flux Rope from Solar Active Region NOAA 11719 to Earth Directed-CME
P. Vemareddy, J. Zhang

TL;DR
This study investigates the initiation and eruption of a magnetic flux rope from solar active region NOAA 11719, linking magnetic field evolution, instability mechanisms, and the resulting Earth-directed CME.
Contribution
It provides detailed analysis of magnetic flux evolution, flux rope dynamics, and instability triggers leading to CME initiation from NOAA 11719.
Findings
Flux rope exhibited kink-rise evolution and increased temperature during eruption.
Magnetic flux cancellation and current increase contributed to flux rope instability.
The eruption was associated with a M6.5 flare and an Earth-directed CME.
Abstract
An eruption event launched from solar active region (AR) NOAA 11719 is investigated based on coronal EUV observations and photospheric magnetic field measurements obtained from Solar Dynamic Observatory. The AR consists of a filament channel originating from major sunspot and its south section is associated with inverse-S sigmoidal system as observed in AIA passbands. We regard the sigmoid as the main body of the flux rope (FR). There also exists a twisted flux bundle crossing over this FR. This overlying flux bundle transforms in shape similar to kink-rise evolution which has correspondence with rise motion of the FR. The emission measure and temperature along the FR exhibits increasing trend with its rising motion, indicating reconnection in the thinning current sheet underneath the FR. Net magnetic flux of the AR evaluated at north and south polarities showed decreasing behavior…
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