Magnetic Field of Solar Dark Filaments Obtained from He I 10830 Angstrom Spectro-polarimetric Observation

Solar filaments are dense and cool plasma clouds in the solar corona. They are supposed to be supported in a dip of coronal magnetic field. However, the models are still under argument between two types of the field configuration; one is the normal polarity model proposed by Kippenhahn & Schluet...

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Veröffentlicht in:	arXiv.org 2023-04
Hauptverfasser:	Yamasaki, Daiki, Yu Wei Huang, Hashimoto, Yuki, Cabezas, Denis P, Kawate, Tomoko, UeNo, Satoru, Ichimoto, Kiyoshi
Format:	Artikel
Sprache:	eng
Schlagworte:	Filaments Magnetic field configurations Magnetic fields Magnetic structure Photosphere Physics - Solar and Stellar Astrophysics Plasma clouds Polarimetry Solar corona Solar magnetic field
Online-Zugang:	Volltext
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