Multiwavelength Observations for a Double-decker Filament Channel in AR 13102
Yin Zhang, Baolin Tan, Quan Wang, Jing Huang, Zhe Xu, Kanfan Ji, Xiao Yang, Jie Chen, Xianyong Bai, Zhenyong Hou, and Yuanyong Deng

TL;DR
This paper provides observational evidence for a double-decker filament channel in active region AR 13102, revealing complex magnetic structures and plasma flows through multiwavelength imaging, enhancing understanding of filament formation and eruption mechanisms.
Contribution
It is the first detailed observational study demonstrating the existence of a double-decker filament channel with complex magnetic and plasma dynamics.
Findings
Confirmed the existence of a double-decker filament channel in AR 13102.
Documented the magnetic reconnection processes and filament interactions.
Observed plasma flows and brightening features associated with filament eruptions.
Abstract
We present the observational evidence of the existence of a double-decker filament channel (FC) by using observations in extreme ultraviolet and H{\alpha} wavelengths. For both FCs, the east foot-point roots in the active region (AR), while the west one roots in the remote quiet region. The bottom FC (FC1) appears as intermittent filaments. Within the AR, the FC1 appears as an S-shaped filament (F1), which consisted of two J-shaped filaments (F1S/F1N for the south/north one). For the upper one (FC2), only the east part is filled with dark plasma and visible as a small filament (F2). Its east foot-point roots around the junction of F1S and F1N. Initially, due to the recurrent reconnections, F1N and F1S link to each other and form a new filament (F3) thread by thread. Meanwhile, the heated plasma, which appears as brightening features, flows from the east foot-point of F2 to the west, and…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Astrophysics and Cosmic Phenomena · Astrophysics and Star Formation Studies
