The Effect of Plasma-β on the Heating Mechanisms during Magnetic Reconnection in Partially Ionized Low Solar Atmosphere

We performed numerical simulations of magnetic reconnection with different strengths of magnetic fields from the solar photosphere to the upper chromosphere. The main emphasis is to identify dominant mechanisms for heating plasmas in the reconnection region under different plasma- β conditions in th...

Täydet tiedot

Bibliografiset tiedot

Päätekijät:	Abdullah Zafar, Lei Ni, Kaifeng Kang, Guanchong Cheng, Jing Ye, Jun Lin, Ahmad Ali, Nadia Imtiaz
Aineistotyyppi:	Artigo
Kieli:	Inglês
Julkaistu:	IOP Publishing 2025-01-01
Sarja:	The Astrophysical Journal
Aiheet:	Solar magnetic reconnection Solar photosphere Magnetohydrodynamical simulations Solar chromosphere
Linkit:	https://doi.org/10.3847/1538-4357/ade714
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