Dependence of Spicule Properties on the Magnetic Field—Results from Magnetohydrodynamics Simulations

Solar spicules are plasma jets observed in the interface region between the visible solar surface and the corona. At any given time, there is a forest of spicules originating in the chromosphere of the Sun. While various models attempt to elucidate their origin and characteristics, here, we consider...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Kartav Kesri, Sahel Dey, Piyali Chatterjee, Robertus Erdelyi
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Solar physics Solar magnetic fields Solar spicules Magnetohydrodynamical simulations Solar atmosphere Radiative magnetohydrodynamics
Online Access:	https://doi.org/10.3847/1538-4357/ad67d8