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机构地区:[1]空军气象学院
出 处:《气象学报》1997年第3期306-317,共12页Acta Meteorologica Sinica
摘 要:本文应用Howard(1961)所用的精巧积分方法研究了三维非静力平衡层结大气随高度变化基流上重力内波的不稳定性质。给出了不稳定产生的必要条件和相速度在相速复平面上的分布规律;发展了Miles定理和Howard半圆定理;得到了有限深度气层的半椭圆定理。并指出在随高度变化的基流中,重力内波的不稳定范围与基流的垂向结构及波传播方向有关;半椭圆的位置和长轴分别重合于Howard半圆的位置和直径,而短轴则依赖于与Richardson数相关的参数J0。By use of the ingenious integral manipulation introduced by Howard(1961), the instability of the basic flow changed with height in three dimensional nonhydrostatic atmosphere has been investigated in the present paper. The essential condition of instability generation and the distribution law of the phase speed on the complex phase speed coodinate plane are explicitely given. Improved Miles theorem and Howard's semicircle theorem, as well as semi ellipse theorem have been established. The semi ellipse theorem means that the complex wave velocity for any unstable mode is restricted in a semi ellipse whose major axis and centre coincide with the diameter and that of Howard's semicircle respectively, and whose minor axis depends not only on the parameters J 0,R 0 associated with the Richardson number and wave number |k| but also on the atmospheric depth parameter k 0 .
关 键 词:变化基流 重力内波 不稳定 半椭圆定理 层结大气
分 类 号:P421.3[天文地球—大气科学及气象学]
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