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- W2023465034 abstract "view Abstract Citations (72) References (27) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Nonaxisymmetric Convection in a Rotating Spherical Shell Durney, B. Abstract The problem of a rotating, convective spherical shell is considered in the Herring approximation. The relevant equations are integrated in time as an initial-value problem. The main results are: 1. The most unstable modes correspond to convective cells stretching from pole to pole. 2. The calculations of the Reynolds stresses show transport of angular momentum toward the equator. That is, differential rotation sets in with equatorial acceleration. 3. The convective transport of heat is maximum at the equator. This would give rise to an equatorpole difference in flux. 4. If convection is nonaxisymmetric (as in the most unstable modes), then there are no time-independent solutions. The time-dependence is oscillatory and of the form A cos (cot + m ) + B sin (cot + m . Publication: The Astrophysical Journal Pub Date: September 1970 DOI: 10.1086/150611 Bibcode: 1970ApJ...161.1115D full text sources ADS |" @default.
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- W2023465034 title "Nonaxisymmetric Convection in a Rotating Spherical Shell" @default.
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