Shallow estuarine basins have small ocean exchange rates during periods of
drought (when they are vertically mixed). This exchange is primarily due to
convective processes. These are forced by a density difference between the
basin and ocean produced by the surface buoyancy flux. This flux is depend
ent on the estuarine temperature, which is itself affected by the ocean exc
hange of heat. This creates a strong interaction between the buoyancy flux,
and the density difference, and may be represented by a Stommel (H. Stomme
l, Tellus. 13 (2) (1961) 224-230) non-linear estuarine model. It involves a
meteorological constant Gamma, and a parameter epsilon, which measures the
strength of the (buoyancy forced) convective exchange processes. The model
has two stable states, or attractors, one of which corresponds to a classi
cal, and the other to an inverse estuary. The analysis considers the range
of (epsilon, Gamma(2)) under which both of these steady states exist and in
vestigates their comparative attractions. On seasonal time scales, the estu
ary may be in a transitory state (described here by manifold theory) in whi
ch the estuary may be 'positive' or 'negative' according to the sign of the
buoyancy flux. For typical meteorological conditions, four categories of t
ransitory estuary emerge which are dependent on the magnitude of epsilon. (
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