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Titlebook: Geophysical Fluid Dynamics; Joseph Pedlosky Book 1982 Springer Science+Business Media New York 1982 Potential.circulation.dynamics.fluid d

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樓主: Sediment
21#
發(fā)表于 2025-3-25 04:58:00 | 只看該作者
Fundamentals, 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.
22#
發(fā)表于 2025-3-25 11:32:02 | 只看該作者
23#
發(fā)表于 2025-3-25 15:25:07 | 只看該作者
24#
發(fā)表于 2025-3-25 18:49:37 | 只看該作者
25#
發(fā)表于 2025-3-25 20:52:56 | 只看該作者
Elektrisches Messen nichtelektrischer Gr??ene persistent but spatially nonuniform solar heating. This input of energy produces a mechanical response, i.e., kinetic energy of the large-scale motion, and eventually this must be dissipated if a steady state—or at least a statistically stable average state of motion—is to be maintained. This requ
26#
發(fā)表于 2025-3-26 03:14:13 | 只看該作者
27#
發(fā)表于 2025-3-26 07:20:16 | 只看該作者
https://doi.org/10.1007/978-3-662-54445-7., that the scaling of the motion is isotropic horizontally. The low-frequency Kelvin wave is not horizontally isotropic, since its offshore scale is the deformation radius, which for low frequencies is small compared with the wavelength. In this chapter we consider some of the refinements to quasig
28#
發(fā)表于 2025-3-26 12:28:32 | 只看該作者
29#
發(fā)表于 2025-3-26 16:16:04 | 只看該作者
Friction and Viscous Flow,e persistent but spatially nonuniform solar heating. This input of energy produces a mechanical response, i.e., kinetic energy of the large-scale motion, and eventually this must be dissipated if a steady state—or at least a statistically stable average state of motion—is to be maintained. This requ
30#
發(fā)表于 2025-3-26 20:26:11 | 只看該作者
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