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- W2002952757 abstract "The hydrodynamic and thermodynamic equations for the upper layers of the ocean are solved by expanding the variables in Fourier series and by making use of the mean field approximation. Solar radiation heating is introduced as a time-dependent source term in the heat conduction equation, and surface cooling processes are represented by a constant heat flux out of the top of the ocean. Wind mixing is represented by eddy coefficients of viscosity and conductivity. The calculations show that convection is inhibited by the solar radiation during the day, but usually soon after sunset the water column became unstable, and convection took place near the sea surface. As night progressed, the convection penetrated more deeply until nearly isothermal conditions in the upper layers prevailed. The convection ceased soon after sunrise. The horizontal spacing of convection cells increased with increasing eddy coefficients. When the eddy coefficients became very large, convection did not take place. The turbidity of the water had only a slight effect on the convection process." @default.
- W2002952757 created "2016-06-24" @default.
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- W2002952757 date "1971-01-20" @default.
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- W2002952757 title "A convective model for the diurnal cycle in the upper ocean" @default.
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- W2002952757 doi "https://doi.org/10.1029/jc076i003p00666" @default.
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