地球大气自转对声-重力波谱的影响

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
O. K. Cheremnykh, S. O. Cheremnykh, D. I. Vlasov
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引用次数: 2

摘要

最近的一项研究[11]表明,考虑到地球大气层的自转,声-重力波诊断图上出现了一个频谱连续的新消去波区域。该区域位于重力波的下限以下,对所有波长都等于\(2\Omega \),其中\(\Omega \)是大气旋转的角频率。这个结果是在大气的高纬度地区得到的,在那里人们可以只考虑地球自转频率的垂直分量。本文表明,考虑到大气旋转频率\(\vec {\Omega }\)矢量\(\vec {\Omega }\)的两个分量——水平分量,\(\Omega \cos \varphi ,\) (\(\varphi \)为当地纬度)和垂直分量,\(\Omega \sin \varphi \)——在声重力波传播中起主导作用的是垂直分量。结果表明,水平分量导致诊断图上声波和重力波区域边界的变化可以忽略不计。频率的垂直分量对重力波的下限影响最大,它取决于观测点的纬度,等于2 \(\Omega \sin \varphi \)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

The Influence of the Earth’s Atmosphere Rotation on the Spectrum of Acoustic-Gravity Waves

The Influence of the Earth’s Atmosphere Rotation on the Spectrum of Acoustic-Gravity Waves

It was shown in a recent study [11] that taking into account the rotation of the Earth’s atmosphere leads to the appearance of a new region of evanescent waves with a continuous frequency spectrum on the diagnostic diagram of acoustic-gravity waves. The region is located below the lower limit of gravity waves, which is equal to \(2\Omega \) for all wavelengths, where \(\Omega \) is the angular frequency of the atmospheric rotation. This result was obtained for high-latitude regions of the atmosphere in which one can be limited to considering only the vertical component of the Earth’s rotation frequency. This paper shows that taking into account both components of the vector \(\vec {\Omega }\) of the atmospheric rotation frequency \(\vec {\Omega }\)—horizontal, \(\Omega \cos \varphi ,\) where \(\varphi \) is the local latitude, and vertical, \(\Omega \sin \varphi \)—the dominant role in the acoustic-gravity wave propagation is played by the vertical component. It is shown that the horizontal component leads to a negligible modification of the boundaries of the regions of acoustic and gravity waves on the diagnostic diagram. It is also shown that the vertical component of the frequency affects most strongly the lower limit of gravity waves, which depends on the latitude of the observation site for all wavelengths and is equal to 2\(\Omega \sin \varphi \).

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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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