2003
DOI: 10.1007/s00032-003-0019-9
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Some Mathematical Aspects of Geophysical Fluid Dynamic Equations

Abstract: In this article we present the classical primitive equations of the ocean, and we summarize a number of results concerning the wellposedness of the associated boundary and initial value problems: some of the results have been known for about ten years or so, and some of the results correspond to very recent results which were proven during the past two years or so. Some indications are also given about the problems of the atmosphere, which are similar, and the coupled ocean and atmosphere.

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Cited by 14 publications
(4 citation statements)
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“…The equations of geophysical fluid dynamics governing the motion of the ocean and the atmosphere are derived from the conservation laws from physics. In the case of a largescale ocean (see, e.g., [10,22,23,26,27,28]), it is considered as made up of a slightly compressible fluid modelled by conservation of momentum and mass equations, with variable density (depending on temperature and salinity) and Coriolis acceleration.…”
Section: Classical Hydrostatic Stokes Formulations In Oceanographymentioning
confidence: 99%
“…The equations of geophysical fluid dynamics governing the motion of the ocean and the atmosphere are derived from the conservation laws from physics. In the case of a largescale ocean (see, e.g., [10,22,23,26,27,28]), it is considered as made up of a slightly compressible fluid modelled by conservation of momentum and mass equations, with variable density (depending on temperature and salinity) and Coriolis acceleration.…”
Section: Classical Hydrostatic Stokes Formulations In Oceanographymentioning
confidence: 99%
“…Also, an asymptotic analysis and the finite‐dimensional behavior of the 3D viscous PEs in a thin domain as the depth of the domain goes to zero were studied in and . For a more extensive discussion and review on this subject, the reader is referred to the recent articles and .…”
Section: Introductionmentioning
confidence: 99%
“…Given a smooth bounded domain M ⊂ R 2 and the cylindrical domain 0 = M × (−h, 0) ⊂ R 3 , consider in 0 the following well known system of 3D viscous Primitive Equations (PEs) of Geophysical Fluid Dynamics (see e.g. [8], [26]- [28], [31,32], [39,40] and the references therein). Conservation of horizontal momentum:…”
mentioning
confidence: 99%
“…Existence and uniqueness of strong solutions, global in time, to the viscous 3D PEs in thin domains for a large set of initial data whose sizes depend inversely on the thickness of the domain were established in [17]. For a more extensive discussion and review on this subject, we refer the reader to the recent articles [39] and [40].…”
mentioning
confidence: 99%