Simulation of a Solar Jet Formed from an Untwisting Flux Rope Interacting with a Null Point

Coronal jets are eruptions identified by a collimated, sometimes twisted spire. They are small-scale energetic events compared with flares. Using multiwavelength observations from the Solar Dynamics Observatory/Atmospheric Imaging Assembly and a magnetogram from Hinode/Spectro-Polarimeter (Hinode/SP...

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Veröffentlicht in:	The Astrophysical journal 2023-05, Vol.949 (1), p.2
Hauptverfasser:	Zhu, Jiahao, Guo, Yang, Ding, Mingde, Schmieder, Brigitte
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Corona Fluctuations Magnetic flux Magnetohydrodynamic simulation Magnetohydrodynamics Photosphere Polarimeters Simulation Solar active regions Solar activity Solar magnetic fields Solar magnetic reconnection Solar observatories
Online-Zugang:	Volltext
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