Convective building of a pycnocline: A two-dimensional nonhydrostatic numerical model

The convective building of a pycnocline is examined using a two-dimensional nonhydrostatic numerical model forced by a balanced salinity dipole (source and sink). Although the forcing fields re steady, the model develops oscillations that renew the model's analog of ''deep waters'' only intermittently. The oscillation cycle consists of a freshwater layer that advects along the surface, capping off the water column under the sense source and preventing sinking; after a time, continuing densification forms a plume that breaks through the salinity barrier and convects beneath the dense source, ventilating the deep water. Increasing the viscosity reduces but does not eliminate this cycle. When the hydrostatic assumption is added, the model evolves systematically different salinity distributions than the nonhydrostatic assumption is added, the model evolves systematically different salinity distributions than the nonhydrostatic model due to the isolation of aprt of the tank by a persistent convective column. The deep flow is also different in this case because of differences between the entrainment/detrainment profile of a hydrostatic plume and one modeled explicity. The model evolves a characteristically skewed distribution of densities that is similar to the distribution of temperature in the World Ocean. Rotation increases the range of this distribution due to the inhibition of meridional flow.