2021
DOI: 10.48550/arxiv.2107.12181
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Formation and Characteristics of Filament Threads in Double-Dipped Magnetic Flux Tubes

Jinhan Guo,
Yuhao Zhou,
Yang Guo
et al.

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 … Show more

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“…Using the observed value of P ≈ 2 hr, the magnetic field strength at the dips is estimated to be ≥34 G, which is consistent with the value for quiescent prominence derived from the flux rope insertion method (e.g. Su & van Ballegooijen 2012;Guo et al 2021).…”
Section: Prominence Seismologysupporting
confidence: 82%
“…Using the observed value of P ≈ 2 hr, the magnetic field strength at the dips is estimated to be ≥34 G, which is consistent with the value for quiescent prominence derived from the flux rope insertion method (e.g. Su & van Ballegooijen 2012;Guo et al 2021).…”
Section: Prominence Seismologysupporting
confidence: 82%