Why are non-radial solar eruptions less frequent than radial ones?

Coronal mass ejections from the Sun are not always initiated along a radial trajectory; such non-radial eruptions are well known to be caused by the asymmetry of the pre-eruption magnetic configuration, which is primarily determined by the uneven distribution of magnetic flux at the photosphere. The...

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Veröffentlicht in:	arXiv.org 2024-06
Hauptverfasser:	Liu, Qingjun, Jiang, Chaowei, Feng, Xuesheng, Zuo, Pingbing, Wang, Yi
Format:	Artikel
Sprache:	eng
Schlagworte:	Asymmetry Coronal mass ejection Current sheets Magnetic flux Photosphere Skewed distributions
Online-Zugang:	Volltext
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