Identification of spectrum of secondary acoustic-gravity waves in the middle and upper atmosphere in a high-resolution numerical model

Pub Date : 2023-09-30 DOI:10.12737/stp-93202310
Nikolay Gavrilov, Sergey Kshevetskii
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Abstract

Considerable attention has recently been paid to the study of so-called “secondary” acoustic-gravity waves (AGWs) that arise as a result of instability and nonlinear interactions of “primary” wave modes propagating from atmospheric sources, among themselves, and with the mean flow. In this paper, for the first time, the horizontal spatial spectra of primary and secondary AGWs are separated at fixed altitude levels in the middle and upper atmosphere at different time moments, which are simulated using a three-dimensional nonlinear high-resolution model AtmoSym. It is shown that in a short time after switching on the plane wave source at the lower boundary of the model, the spectrum consists of a peak corresponding to primary AGW and quasi-white noise generated by random atmospheric disturbances and the numerical model. Later, secondary peaks appear in the spectra at horizontal wave numbers, which are multiples of the wave numbers of primary AGW. The proposed separation of the spectra of primary and secondary AGWs makes it possible to estimate the relative contribution of secondary AGW at different altitudes, at different times, and with different stability of background temperature and wind profiles in the atmosphere.
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中高层大气二次声重波谱的高分辨率数值模式识别
最近,人们对所谓的“二次”声重力波(AGWs)的研究给予了相当大的关注,这种波是由于从大气源传播的“初级”波模式之间以及与平均流之间的不稳定性和非线性相互作用而产生的。本文首次在中、高层大气固定高度分离了主、次AGWs在不同时间时刻的水平空间光谱,利用三维非线性高分辨率模式AtmoSym对其进行了模拟。结果表明,在模式下边界打开平面波源后的短时间内,谱由一个与主AGW对应的峰以及随机大气扰动和数值模式产生的准白噪声组成。随后,在水平波数处出现二次峰,这些波数是一次AGW波数的倍数。将主、次AGW的光谱分离,可以估算不同高度、不同时间、不同背景温度和风廓线稳定性下的次AGW的相对贡献。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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