Formation and Characteristics of Filament Threads in Double-Dipped Magnetic Flux Tubes
Jinhan Guo, Yuhao Zhou, Yang Guo, Yiwei Ni, Judy Karpen, Pengfei Chen

TL;DR
This study uses numerical simulations to explore how filament threads form in double-dipped magnetic flux tubes, revealing conditions that favor their formation and explaining features of quiescent filaments.
Contribution
It introduces a novel analysis of filament formation in double-dipped flux tubes, extending the evaporation-condensation model beyond single-dip configurations.
Findings
Magnetically connected threads are more common in quiescent filaments.
Formation requires specific magnetic configurations and localized heating.
Threads in double-dipped tubes are shorter, explaining filament features.
Abstract
As one of the main formation mechanisms of solar filament formation, the chromospheric evaporation-coronal condensation model has been confirmed by numerical simulations to explain the formation of filament threads very well in flux tubes with single dips. However, coronal magnetic extrapolations indicated that some magnetic field lines might possess more than one dip. It is expected that the formation process would be significantly different in this case compared to a single-dipped magnetic flux tube. In this paper, based on the evaporation-condensation model, we study filament thread formation in double-dipped magnetic flux tubes by numerical simulations. We find that only with particular combinations of magnetic configuration and heating, e.g., concentrated localized heating and a long magnetic flux tube with deep dips, can two threads form and persist in a double-dipped magnetic…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
