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KIRK BRYAN IS an American oceanographer and Senior Research Scholar at Princeton University whose research has dealt with the construction of models for ocean circulation and the roles played by oceans in the climate system. Bryan is considered the founder of numerical ocean modeling. Climate models are computer-based simulations that use mathematical formulas to recreate the chemical and physical processes that drive Earth's climate. Bryan's original model is still considered an insight of enormous importance for climate science and weather forecasting. Earlier knowledge of the oceanic and atmospheric circulation, and their interactions, was based purely on theory and observation.

According to Bryan, the world's oceans are one of the least-understood elements in the climate system. His research aims to understand the role of ocean circulation in the Earth's current climate, and its variations over the recent geological record. To gain a better understanding of ocean circulation, Bryan has systematically compared data and has established a hierarchy of coupled models of increasing complexity. Bryan's work is geared toward a comparison of the atmosphere and the ocean, and their roles in the global heat and water balance.

The Bryan-Cox Code

Bryan started his research at the Geophysical Fluid Dynamics Laboratory in the 1960s. The laboratory was then located in Washington, D.C. (it has since transferred to Princeton University). With a team of colleagues, Bryan developed numerical schemes to calculate the equations of motion describing flow on a sphere. These schemes led to the “Bryan-Cox code,” used in many early simulations, which allowed the development of the Modular Ocean Model currently used by many numerical oceanographers and climate scientists.

The “Bryan-Cox code” was used to create the first simulation models that calculate realistic circulation of oceanic regions. The models are often very complex, and their output is difficult to interpret. The Bryan-Cox model calculated the three-dimensional flow in the ocean combining the continuity and momentum equation with the hydrostatic and Bouss-inesq approximations, and a simplified equation of state. These models are called primitive equation models because they use the most basic form of the equations of motion. The equation of state allows the model to calculate changes in density due to fluxes of heat and water through the sea surface, so the model includes thermodynamic processes.

The Bryan-Cox model used large horizontal and vertical viscosity and diffusion to eliminate turbulent eddies of diameters smaller than about 311 mi. (500km.). It also had complex coastlines, smoothed sea-floor features, and a rigid lid. The rigid lid was necessary for eliminating ocean-surface waves, such as tides and tsunamis, which move far too fast to be accounted for by the time steps used by all simulation models. Criticism of the model concerns the lid. Islands substantially slow the computation, and the sea-floor features must be smoothed to eliminate steep gradients.

The Geophysical Fluid Dynamics Laboratory Modular Ocean Model (MOM) is perhaps the most widely used model that grew out of the original Bryan-Cox code. It is made up of a large set of modules that can be configured to run on many different computers to model many different aspects of the circulation. The source code is open and free. The model is commonly used for climate studies and to assess the ocean's circulation over a wide range of space and time scales. The Parallel Ocean Program Model also grew out of the Bryan-Cox code.

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