Hydrodynamics of the equatorial ocean - ISBN:0444421963

Hydrodynamics of the equatorial ocean

Date: 23 April 2011, 23:46

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The study of sea surface temperature (SST) variability in the equatorial oceans is of great value to physical oceanographers and atmospheric scientists alike. Aside from an interest in simply documenting and describing equatorial SST, oceanographers often use SST as a tracer for subsurface dynamical phenomena that are either too difficult or too expensive to observe directly. For example, the accumulation of warm water off the coast of Peru has often been interpreted as evidence for the existence of equatorial Kelvin waves (e.g. McCreary, 1976). Likewise, Moore & e. (1978) have hypothesized that cold SST in the Gulf of Guinea during coastal upwelling season is the result of a coastal Kelvin wave, which through a complex series of events involving equatorial waves, is excited by changing winds in the western equatorial Atlantic. The physical basis for this dynamical influence on SST is that when cold thermocline water is brought closer to (further from) the surface, it is easier (harder) to mix across the base of the mixed layer.

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