Rapid Changes of Photospheric Magnetic Field after Tether-Cutting Reconnection and Magnetic Implosion
Chang Liu, Na Deng, Rui Liu, Jeongwoo Lee, Thomas Wiegelmann, Ju Jing,, Yan Xu, Shuo Wang, and Haimin Wang

TL;DR
This study investigates rapid photospheric magnetic field changes during a solar flare, linking them to tether-cutting reconnection and magnetic implosion through multi-instrument observations and NLFFF modeling.
Contribution
It provides detailed analysis of magnetic field evolution during a flare, highlighting the role of tether-cutting reconnection and coronal field implosion.
Findings
28% increase in horizontal magnetic field strength in the flare region
Coronal currents collapsed downward after the sigmoid eruption
Magnetic field changes are consistent with tether-cutting reconnection and implosion models
Abstract
The rapid, irreversible change of the photospheric magnetic field has been recognized as an important element of the solar flare process. This Letter reports such a rapid change of magnetic fields during the 2011 February 13 M6.6 flare in NOAA AR 11158 that we found from the vector magnetograms of the Helioseismic and Magnetic Imager with 12-min cadence. High-resolution magnetograms of Hinode that are available at ~-5.5, -1.5, 1.5, and 4 hrs relative to the flare maximum are used to reconstruct three-dimensional coronal magnetic field under the nonlinear force-free field (NLFFF) assumption. UV and hard X-ray images are also used to illuminate the magnetic field evolution and energy release. The rapid change is mainly detected by HMI in a compact region lying in the center of the magnetic sigmoid, where the mean horizontal field strength exhibited a significant increase by 28%. The…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
