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• W1991330386 startingPage "L61" @default.
• W1991330386 abstract "The layer of transition from the nearly rigid rotation of the radiative interior to the latitudinal differential rotation of the convection zone plays a significant role in the internal dynamics of the Sun. Using rotational splitting coefficients of the p-mode frequencies, obtained during 1986-1990 at the Big Bear Solar Observatory, we have found that the thickness of the transitional layer is 0.09 ± 0.04 solar radii (63 ± 28 Mm), and that most of the transition occurs beneath the adiabatically stratified part of the convection zone, as suggested by the dynamo theories of the 22 yr solar activity cycle." @default.
• W1991330386 created "2016-06-24" @default.
• W1991330386 creator A5055414639 @default.
• W1991330386 date "1996-09-20" @default.
• W1991330386 modified "2023-09-23" @default.
• W1991330386 title "Helioseismic Constraints on the Gradient of Angular Velocity at the Base of the Solar Convection Zone" @default.
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• W1991330386 doi "https://doi.org/10.1086/310253" @default.
• W1991330386 hasPublicationYear "1996" @default.
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