Sigmoid Formation Through Slippage of A Single J-shaped Coronal Loop
Hanya Pan, Tingyu Gou, Rui Liu

TL;DR
This study demonstrates that a single J-shaped coronal loop can transform into an S-shaped sigmoid through rapid slipping reconnection, highlighting a new pathway for sigmoid formation in solar eruptions.
Contribution
It provides observational evidence for sigmoid formation via slipping reconnection of a single loop, differing from traditional models involving double loops.
Findings
Loop slips at speeds over 1000 km/s during formation.
Heating occurs in the slipping loop segment.
Coronal emission dims due to loop lengthening and heating.
Abstract
A well-known precursor of an imminent solar eruption is the appearance of a hot S-shaped loop, also known as sigmoid, in an active region (AR). Classically, the formation of such an S-shaped loop is envisaged to be implemented by magnetic reconnection of two oppositely oriented J-shaped loops. However, the details of reconnection are elusive due to weak emission and subtle evolution during the pre-eruptive phase. In this paper, we investigate how a single J-shaped loop transforms into an S-shaped one through the slippage of one of its footpoints in NOAA AR 11719 on 2013 April 11. During an interval of about 16 min, the J-shaped loop slips through a low-corona region of strong electric current density in a bursty fashion, reaching a peak apparent speed as fast as over 1000 km s, at the slipping footpoint. The enhancement of electric current density, as suggested by non-linear…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Geomagnetism and Paleomagnetism Studies
