標題: Titlebook: Geophysical Fluid Dynamics; Joseph Pedlosky Book 19791st edition Springer Science+Business Media New York 1979 Dissipation.dynamics.fluid [打印本頁] 作者: 民俗學 時間: 2025-3-21 19:10
書目名稱Geophysical Fluid Dynamics影響因子(影響力)
書目名稱Geophysical Fluid Dynamics影響因子(影響力)學科排名
書目名稱Geophysical Fluid Dynamics網絡公開度
書目名稱Geophysical Fluid Dynamics網絡公開度學科排名
書目名稱Geophysical Fluid Dynamics被引頻次
書目名稱Geophysical Fluid Dynamics被引頻次學科排名
書目名稱Geophysical Fluid Dynamics年度引用
書目名稱Geophysical Fluid Dynamics年度引用學科排名
書目名稱Geophysical Fluid Dynamics讀者反饋
書目名稱Geophysical Fluid Dynamics讀者反饋學科排名
作者: 滲入 時間: 2025-3-21 23:49 作者: Encoding 時間: 2025-3-22 01:19 作者: cyanosis 時間: 2025-3-22 07:40
Ageostrophic Motion,., 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作者: 暫時別動 時間: 2025-3-22 11:58
https://doi.org/10.1007/978-3-642-50943-8s of years, the surface expression of which is sea-floor spreading and continental drift. All these phenomena can properly be included within the domain of geophysical fluid dynamics. Partly for historical reasons, however, the subject has tended to focus on the dynamics of large-scale phenomena in 作者: Employee 時間: 2025-3-22 16:49
https://doi.org/10.1007/978-3-642-25794-0the 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 re作者: Employee 時間: 2025-3-22 19:57 作者: 全神貫注于 時間: 2025-3-22 23:41 作者: 修正案 時間: 2025-3-23 03:21 作者: 萬靈丹 時間: 2025-3-23 07:37
0172-6234 s curriculum were merely classical rather than essential and could be, however sadly, dispensed with for our purposes. At the same time, the diversity of interests of our students is so great that no curriculum can truly be exhaust- ive in such a curriculum period. It seems to me that the best that can be ach978-1-4684-0071-7Series ISSN 0172-6234 作者: 迅速成長 時間: 2025-3-23 12:56 作者: 割公牛膨脹 時間: 2025-3-23 17:06 作者: 暗指 時間: 2025-3-23 21:18
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作者: CANDY 時間: 2025-3-24 02:14
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作者: faddish 時間: 2025-3-24 03:47
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作者: curriculum 時間: 2025-3-24 09:38
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作者: 自負的人 時間: 2025-3-24 12:42 作者: Narrative 時間: 2025-3-24 15:09
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作者: Myelin 時間: 2025-3-24 22:30
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.作者: 指數(shù) 時間: 2025-3-25 02:05 作者: LIEN 時間: 2025-3-25 04:06
https://doi.org/10.1007/978-1-4684-0071-7Dissipation; dynamics; fluid dynamics; fluid- and aerodynamics作者: colostrum 時間: 2025-3-25 07:49
Springer Science+Business Media New York 1979作者: FAR 時間: 2025-3-25 14:36
Geophysical Fluid Dynamics978-1-4684-0071-7Series ISSN 0172-6234 作者: 抒情短詩 時間: 2025-3-25 16:29
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作者: 廚房里面 時間: 2025-3-25 21:22 作者: 愛得痛了 時間: 2025-3-26 01:49
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作者: Shuttle 時間: 2025-3-26 08:13
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作者: flammable 時間: 2025-3-26 11:56
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作者: 小木槌 時間: 2025-3-26 13:12
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作者: ODIUM 時間: 2025-3-26 20:24
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作者: 清晰 時間: 2025-3-27 00:42 作者: 檢查 時間: 2025-3-27 02:29
Book 19791st editionhysical Sciences at The University of Chicago have taught for the past decade. Our purpose in developing a core curriculum was to provide to advanced undergraduates and entering graduate students a coherent and systematic introduction to the theory of geophysical fluid dynamics. The curriculum and t作者: 誘拐 時間: 2025-3-27 07:48 作者: NEEDY 時間: 2025-3-27 13:25 作者: travail 時間: 2025-3-27 17:07 作者: Insulin 時間: 2025-3-27 20:21 作者: 大氣層 時間: 2025-3-28 01:47 作者: placebo 時間: 2025-3-28 04:05 作者: Sarcoma 時間: 2025-3-28 08:24 作者: Atheroma 時間: 2025-3-28 11:46 作者: Malleable 時間: 2025-3-28 17:45 作者: 地名表 時間: 2025-3-28 20:37
Stephen D. Brookes one gets immediately trapped by the breathtaking beauty of the op- calimagestakenfromEarthorSpacewithmoderntelescopes,onlytodiscover soonafterthatthephysicsthatregulatestheirpropertiesisevenmoreintri- ing. Out?ows are believed to play a fundamental role in the formationprocess of a new star and its作者: Instrumental 時間: 2025-3-29 01:00
