Titlebook: Geophysical Fluid Dynamics; Joseph Pedlosky Book 19791st edition Springer Science+Business Media New York 1979 Dissipation.dynamics.fluid

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https://doi.org/10.1007/978-3-663-09909-3oses to our consideration of this physical system. It is first of all simple enough so that the issues raised by the problem of geostrophic degeneracy can be dealt with directly without the need to simultaneously treat the complexities of the thermodynamics of a density-stratified fluid. The first g

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https://doi.org/10.1007/978-3-642-25794-0weak, almost everywhere, when compared with the Coriolis acceleration and the pressure gradient. Friction rarely upsets the geostrophic balance to lowest order. Indeed, for many flows it is probably also true that the dissipa-tive time scale is long compared to the advective time scale, i.e., that t

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Elektrische und magnetische Felderare the dramatic elements of many a sea story. With the advent of the great age of navigation and exploration a more systematic description of the general pattern of the oceanic circulation began to emerge. It is clear now that a time-averaged circulation pattern exists in all oceans, although its o

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Elektrische und magnetische Felderrculations of both systems. Even the wind-driven oceanic circulation implicitly requires atmospheric buoyancy forces to produce the wind. In addition, the presence of a stable stratification in which heavier fluid underlies lighter, characteristic of both the atmosphere and the oceans, inhibits vert

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https://doi.org/10.1007/978-3-642-48064-5ion that the time scale of the motion is large compared to ... This is not always sufficient, as the discussion of the Kelvin wave in Section 3.9 indicated. When the wavelength of the Kelvin wave is long compared to the deformation radius, the frequency is small compared to .. Yet the equation of mo

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https://doi.org/10.1007/978-3-0348-6551-7 any particular problem. However, the equations of motion are so complex that only rarely can exact solutions be found, and any method of approximation of the equations requires first an understanding of the broad, general, physical principles with which any approximation must be consistent.

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