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/10.1007/978-1-4684-0071-7Dissipation; dynamics; fluid dynamics; fluid- and aerodynamics

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Springer Science+Business Media New York 1979

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Geophysical Fluid Dynamics978-1-4684-0071-7Series ISSN 0172-6234

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Preliminaries,perience has also shown that the recognition of the underlying dynamical concepts applicable to both the atmosphere and the oceans is an excellent starting point for the study of either. Geophysical fluid dynamics is the subject whose concerns are the fundamental dynamical concepts essential to an u

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Inviscid Shallow-Water Theory,oses 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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Friction and Viscous Flow,weak, 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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Homogeneous Models of the Wind-Driven Oceanic Circulation,are 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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Quasigeostrophic Motion of a Stratified Fluid on a Sphere,rculations 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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Instability Theory, The radiant energy emitted by the sun may vary somewhat over very long periods, but a sensible idealization for most meteorological and oceanographic purposes consists in considering the solar source strength as fixed. Temporal variations in the incident radiation (and its spatial distribution) are