Comprehensive Radiative MHD Simulations of Eruptive Flares above Collisional Polarity Inversion Lines

We present a new simulation setup using the MURaM radiative MHD code that allows the study of the formation of collisional polarity inversion lines (cPILs) in the photosphere and the coronal response including flares. In this scheme, we start with a bipolar sunspot configuration and set the spots on...

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Veröffentlicht in:	The Astrophysical journal 2023-10, Vol.955 (2), p.105
Hauptverfasser:	Rempel, Matthias, Chintzoglou, Georgios, Cheung, Mark C. M., Fan, Yuhong, Kleint, Lucia
Format:	Artikel
Sprache:	eng
Schlagworte:	Active solar corona Astrophysics Collision dynamics Corona Coronal mass ejection Flares Inversion Magnetic flux Photosphere Physical properties Polarity Radiative magnetohydrodynamics Simulation Solar active region magnetic fields Solar active regions Solar coronal mass ejections Solar flares Solar photosphere Sunspots Velocity distribution
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