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地转气流中的重力惯性内波
引用本文:巢纪平,吴钦岳. 地转气流中的重力惯性内波[J]. 气象学报, 1964, 34(4): 523-530
作者姓名:巢纪平  吴钦岳
作者单位:中国科学院地球物理研究所(巢纪平),中国科学技术大学(吴钦岳)
摘    要:本文用一个一维线性的二层模式,分析了地转气流中重力惯性内波的动力学性质。讨论了重力惯性内波的不稳定性、相速度和群速度后,指出: 1)当地转风速大于重力内波波速时,某些尺度的重力惯性内波可以产生不稳定性,这种不稳定性可以用来解释某些中系统的发展。 2)某些波长的重力惯性内波,它的群速度可以大于相速度;因此在某一地区有中系统发展时,它的能量可以很快地传到下游,而在某下游产生新的系统。


SOME ASPECTS ON THE GRAVITATIONAL WAVES IN A GEOSTROPHIC CURRENTS
CHAO JIH-PING and WU QING-YU. SOME ASPECTS ON THE GRAVITATIONAL WAVES IN A GEOSTROPHIC CURRENTS[J]. Acta Meteorologica Sinica, 1964, 34(4): 523-530
Authors:CHAO JIH-PING and WU QING-YU
Affiliation:Institute of Geophysics and Meteorology, Academia Sinica;The Chinese University of Science and Technology
Abstract:In this paper,the instability,phase velocity and group velocity of the gravitational waves in a geostrophic currents arc analysed by using a two layer model.The conclusions reached arc that:1.When the Froude number is greater than unit,the gravitational waves of some wave lengths will become unstable.This instability may be used to explain the development of some meso-scale systems.2.The group velocity of the gravitational waves can exceed its phase velocity.Therefore,when a meso-scale system is developed in some regions,its energy can travel faster downwind than the phase velocity,therefore a new wave may be formed in the front of the old one.
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