Magnetohydrodynamic Instabilities of Double Magnetic Bands in a Shallow-water Tachocline Model. II. Teleconnection Between High- and Low-latitude Bands and Across Equator

The “extended solar cycle” indicates that there are two deeply seated toroidal magnetic field bands in each hemisphere. Both bands migrate equatorward as a sunspot cycle progresses. Here, we examine the consequences of global MHD instability of this migrating double-band system in tachocline on the...

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Egile Nagusiak:	Mausumi Dikpati, Bernadett Belucz, Robertus Erdélyi, Peter A. Gilman, Scott W. McIntosh, Breno Raphaldini
Formatua:	Artigo
Hizkuntza:	Inglês
Argitaratua:	IOP Publishing 2024-01-01
Saila:	The Astrophysical Journal
Gaiak:	Solar activity Magnetohydrodynamics Solar interior Solar photosphere Solar cycle
Sarrera elektronikoa:	https://doi.org/10.3847/1538-4357/ad8b50
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