Self-similar Solutions of Oscillatory Reconnection: Parameter Study of Magnetic Field Strength and Background Temperature

Oscillatory reconnection is a specific type of time-dependent reconnection which involves periodic changes in the magnetic topology of a null point. The mechanism has been reported for a variety of magnetic field strengths and configurations, background temperatures, and densities. All these studies...

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Autori principali:	Luiz A. C. A. Schiavo, Gert J. J. Botha, James A. McLaughlin
Natura:	Artigo
Lingua:	Inglês
Pubblicazione:	IOP Publishing 2024-01-01
Serie:	The Astrophysical Journal
Soggetti:	Solar magnetic reconnection Solar physics Solar coronal transients Solar coronal heating Magnetohydrodynamics
Accesso online:	https://doi.org/10.3847/1538-4357/ad7600
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