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Titlebook: Atmospheric Tidal and Planetary Waves; Hans Volland Book 1988 Kluwer Academic Publishers 1988 Scale.Southern Oscillation.Storm.Tide.wind

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樓主
發(fā)表于 2025-3-21 18:28:19 | 只看該作者 |倒序瀏覽 |閱讀模式
期刊全稱Atmospheric Tidal and Planetary Waves
影響因子2023Hans Volland
視頻videohttp://file.papertrans.cn/165/164651/164651.mp4
發(fā)行地址Includes supplementary material:
學(xué)科分類Atmospheric and Oceanographic Sciences Library
圖書封面Titlebook: Atmospheric Tidal and Planetary Waves;  Hans Volland Book 1988 Kluwer Academic Publishers 1988 Scale.Southern Oscillation.Storm.Tide.wind
影響因子Prior to the space age, meteorologists rarely paid particular attention to the height regions above the tropopause. What was known about the upper atmosphere above about 100 km came essentially from ionospheric and geomagnetic research. The region in between, presently known as the middle atmosphere, was almost terra incognita above the height reachable by balloons. It was space research that allowed for the first time direct access to middle and upper atmospheric heights. About 40 years ago, Sidney Chapman coined a new word ‘a(chǎn)eronomy‘ to describe the study of these two height regions. When asked about the difference between aeronomy and meteorology, he allegedly replied: ‘it is the same as between astronomy and astrology‘ . This mild irony indicates the preferred prejudice of many ionospheric physicists and geomagneticians in those days toward meteorology as a descriptive rather than an exact science, in spite of the presence of such giants as Carl Rossby and Hans Ertel.
Pindex Book 1988
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沙發(fā)
發(fā)表于 2025-3-21 20:48:04 | 只看該作者
https://doi.org/10.1007/978-94-007-7091-1at the equations of motion can be solved by separation of the variables (latitude, longitude, height, and time) and that the modal structure becomes an eigenvalue problem. In this chapter, we will discuss the eigenvalues of the individual modes and their horizontal structures.
板凳
發(fā)表于 2025-3-22 04:27:44 | 只看該作者
地板
發(fā)表于 2025-3-22 08:19:22 | 只看該作者
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發(fā)表于 2025-3-22 10:24:31 | 只看該作者
Horizontal Modal Structure,at the equations of motion can be solved by separation of the variables (latitude, longitude, height, and time) and that the modal structure becomes an eigenvalue problem. In this chapter, we will discuss the eigenvalues of the individual modes and their horizontal structures.
6#
發(fā)表于 2025-3-22 14:48:36 | 只看該作者
7#
發(fā)表于 2025-3-22 18:56:25 | 只看該作者
Book 1988 indicates the preferred prejudice of many ionospheric physicists and geomagneticians in those days toward meteorology as a descriptive rather than an exact science, in spite of the presence of such giants as Carl Rossby and Hans Ertel.
8#
發(fā)表于 2025-3-22 23:34:07 | 只看該作者
9#
發(fā)表于 2025-3-23 04:41:02 | 只看該作者
Internal Energy Sources and Sinks,bypass these difficulties by introducing secondary or internal ‘sources’ (or ‘sinks’). These internal sources are intended to parameterize the otherwise neglected processes like turbulence, latent heat, feedback between ground and atmosphere, etc.
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發(fā)表于 2025-3-23 06:28:07 | 只看該作者
Nonlinear Wave Propagation,e types with mixed frequencies. Such interference cannot be described by the linear approximation. We want to estimate in this chapter the influence of the nonlinear terms in the wave equations on the excitation and propagation of global-scale waves.
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