等温大气中的波扰动频谱因旋转而分裂

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2023-12-02 DOI:10.3103/S0884591323060028
O. K. Cheremnykh, A. K. Fedorenko, S. O. Cheremnykh, O. O. Kronberg
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引用次数: 0

摘要

研究了地球自转对等温大气中低频波扰动频谱的影响。根据 "传统 "近似和 β 平面近似,并考虑到大气的旋转频率,得到了小线性扰动的方程组。所发现的方程与之前得到的方程不同,方程的左侧部分只取决于时间,而右侧部分则用扰动压力表示。研究表明,在扰动压力为零时,在方程中考虑大气旋转会导致所得到的系统 "分裂 "为描述垂直和水平扰动的独立方程。对于这两种扰动,都获得了紧凑的分析解。结果表明,垂直扰动以 Brunt-Väisälä 波的形式实现,而水平扰动则以 Rossby 波和惯性振荡的形式实现。
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Splitting of the Wave Disturbance Spectrum in the Isothermal Atmosphere Due to Its Rotation

The influence of the Earth’s rotation on the spectrum of low-frequency wave disturbances in an isothermal atmosphere is investigated. The system of equations for small linear disturbances is obtained in the “traditional” approximation and in the β-plane approximation, taking into account the frequency of rotation of the atmosphere. The found equations differ from the previously obtained ones in that the left parts of the equations depend only on time, whereas the right parts are expressed in terms of disturbed pressure. It is shown that, at zero perturbed pressure, taking into account the atmospheric rotation in the equations leads to the “splitting” of the obtained system into separate equations describing vertical and horizontal perturbations. Compact analytical solutions were obtained for both types of disturbances. It was established that vertical disturbances are realized in the form of Brunt–Väisälä waves, while horizontal are realized in the form of Rossby waves and inertial oscillations.

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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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