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The rotating shallow water (RSW) model is of wide use as a
conceptual tool in geophysical fluid dynamics (GFD), because, in
spite of its simplicity, it contains all essential ingredients of
atmosphere and ocean dynamics at the synoptic scale, especially in
its two- (or multi-) layer version. The book describes recent
advances in understanding (in the framework of RSW and related
models) of some fundamental GFD problems, such as existence of the
slow manifold, dynamical splitting of fast (inertia-gravity waves)
and slow (vortices, Rossby waves) motions, nonlinear geostrophic
adjustment and wave emission, the role of essentially nonlinear
wave phenomena. The specificity of the book is that analytical,
numerical, and experimental approaches are presented together and
complement each other. Special attention is paid on explaining the
methodology, e.g. multiple time-scale asymptotic expansions,
averaging and removal of resonances, in what concerns theory,
high-resolution finite-volume schemes, in what concerns numerical
simulations, and turntable experiments with stratified fluids, in
what concerns laboratory simulations. A general introduction into
GFD is given at the beginning to introduce the problematics for
non-specialists. At the same time, recent new results on nonlinear
geostrophic adjustment, nonlinear waves, and equatorial dynamics,
including some exact results on the existence of the slow manifold,
wave breaking, and nonlinear wave solutions are presented for the
first time in a systematic manner.
Geophysical fluid dynamics examines the dynamics of stratified and turbulent motion of fluids in the ocean and outer core, and of gases in the atmosphere. This book explains key notions and fundamental processes of the dynamics of large- and medium-scale atmospheric and oceanic motions from the unifying viewpoint of the rotating shallow water model. The model plays a distinguished role in geophysical fluid dynamics. It has been used for about a century for conceptual understanding of various phenomena, for elaboration of approaches and methods to be used later in more complete models, for development and testing of numerical codes, and for many other purposes. In spite of its simplicity, the model grasps essential features of the complete "primitive equations" models, being their vertically averaged version, and gives an intuitive representation and clear vision of principal dynamical processes. This book is a combination of a course on geophysical fluid dynamics (Part 1), with explanations and illustrations of fundamentals, and problems, as well as a more advanced treatise of a range of principal dynamical phenomena (Part 2), including recently arisen approaches and applications (Part 3). Mathematics and physics underlying dynamical phenomena are explained, with necessary demonstrations. Yet, an important goal of the book is to develop the reader's physical intuition and qualitative insights.
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