Measurements of the Magnetic Field Strengths at the Bases of Stellar Coronae Using the Magnetic-field-induced Transition Theory

Measurements of the magnetic field in the stellar coronae are extremely difficult. Recently, it was proposed that the magnetic-field-induced transition (MIT) of the Fe x 257 Å line can be used to measure the coronal magnetic field of the Sun. We performed forward modeling with a series of global ste...

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Veröffentlicht in:	Astrophysical journal. Letters 2021-09, Vol.918 (1), p.L13
Hauptverfasser:	Chen, Yajie, Liu, Xianyu, Tian, Hui, Bai, Xianyong, Jin, Meng, Li, Wenxian, Yang, Yang, Yang, Zihao, Deng, Yuanyong
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Computational fluid dynamics Coronal magnetic fields Flux density Magnetic fields Magnetic flux Magnetism Magnetohydrodynamics Modelling Stellar coronae Stellar coronas Stellar magnetic fields Stellar models
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