Acoustic Gravity Waves with Height-Independent Amplitude in the Isothermal Atmosphere

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
O. K. Cheremnykh, A. K. Fedorenko, S. O. Cheremnykh, E. A. Kronberg
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Abstract

Acoustic gravity wave modes in the Earth’s thermosphere, the amplitude of which does not depend on height, are theoretically investigated. These studies are stimulated by satellite observations, according to which the amplitudes of acoustic gravity waves in the polar thermosphere do not show dependence on height in the altitude range of 250–450 km. It is shown that the propagation of acoustic gravity wave modes with the height-independent amplitude should be considered as an oscillatory process that occurs simultaneously at two natural frequencies. The dispersion equation for these waves is obtained. According to the frequency–wave vector diagnostic diagram, the dispersion dependence of waves with the constant amplitude is in the region that is prohibited for free propagation. It separates the waves propagating horizontally, in which the amplitude in the vertical direction increases from waves with the amplitude decreasing in the vertical direction. Solutions are found for the perturbed quantities in the two-frequency mode of oscillations. It is noted that the superposition of a few of such modes can lead to the emergence of complex resulting motions close to turbulent ones. It is shown that there is a selected quasi-harmonic mode with the constant amplitude, which is characterized by a fixed frequency and wavelength. It is concluded that this kind of wave mode with the height-independent amplitude of the perturbed values prevails in the observations in the Earth’s polar thermosphere.

Abstract Image

等温大气中振幅与高度无关的重力声波
从理论上研究了地球热层中的声波重力波模式,其振幅与高度无关。这些研究受到卫星观测的刺激,根据卫星观测,极地热层中重力声波的振幅在250–450公里的高度范围内不显示出对高度的依赖性。结果表明,具有高度无关振幅的声重力波模式的传播应被视为在两个固有频率下同时发生的振荡过程。得到了这些波的色散方程。根据频率-波矢量诊断图,具有恒定振幅的波的色散依赖性处于禁止自由传播的区域。它将水平传播的波从垂直方向振幅减小的波中分离出来,其中垂直方向振幅增大。找到了双频振荡模式下扰动量的解。值得注意的是,其中一些模式的叠加可能会导致出现接近湍流的复杂运动。结果表明,存在一个选定的具有恒定振幅的准谐波模式,其特征是固定的频率和波长。结果表明,在地球极地热层的观测中,这种扰动值振幅与高度无关的波动模式普遍存在。
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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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