The Response of Rotating Stellar Convection to Latitudinally Varying Heat Flux

We investigate how rotating convection responds to the imposition of a latitudinally varying heat flux at the base of the convective layer. This study is motivated by the solar near-surface shear layer, whose flows are thought to transition from a buoyancy-dominated regime near the photosphere to a...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής

Κύριοι συγγραφείς:	Kinfe Teweldebirhan, Rituparna Curt, Nicholas A. Featherstone
Μορφή:	Artigo
Γλώσσα:	Inglês
Έκδοση:	IOP Publishing 2026-01-01
Σειρά:	The Astrophysical Journal
Θέματα:	Solar interior Solar convective zone Stellar convective zones Hydrodynamics Solar differential rotation Astrophysical fluid dynamics
Διαθέσιμο Online:	https://doi.org/10.3847/1538-4357/ae28d0
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