Seasonal Features of the Spatial Distribution of Atmospheric Gravity Waves in the Earth’s Polar Thermosphere

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2022-05-18 DOI:10.3103/S0884591322020076
D. I. Vlasov, A. K. Fedorenko, E. I. Kryuchkov, O. K. Cheremnykh, I. T. Zhuk
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Abstract

The features of the spatial distribution of atmospheric gravity waves (AGW) in the polar thermosphere of the Earth are investigated. The research is based on data from direct satellite measurements of the parameters of the neutral atmosphere. According to satellite data, the amplitudes of AGWs that are systematically observed in the polar regions of both hemispheres are usually several times higher than the amplitudes of these waves in the middle and low latitudes. At the same time, the polar AGWs of large amplitudes are recorded against the background of high-speed spatially inhomogeneous wind flows, which indicates their possible amplification caused by interaction with the wind. Based on the analysis of measurement data on the Dynamics Explorer 2 satellite, the relationship between the spatial distribution of the atmospheric gravitational waves and the auroral oval has been revealed. On a large volume of experimental data, seasonal patterns of the distribution of the wave field over the Antarctic and the Arctic have been established. A comparative analysis of the features of the AGWs in the polar thermosphere of both hemispheres for the conditions of the polar day and polar night has been carried out. Some differences in the distribution of the AGWs were noted depending on the Kp-index. It has been suggested that the observed seasonal features of the AGW distribution and its dependence on the level of geomagnetic activity are associated with the restructuring of the polar wind circulation when the conditions of solar illumination and geomagnetic conditions change.

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地球极地热层大气重力波空间分布的季节特征
研究了地球极地热层大气重力波的空间分布特征。这项研究是基于对中性大气参数的直接卫星测量数据。根据卫星资料,在两个半球两极地区系统观测到的agw振幅通常比中低纬度地区的agw振幅高几倍。同时,在高速空间非均匀风的背景下,记录了大振幅的极极AGWs,表明其可能由于风的相互作用而放大。通过对动力学探索者2号卫星测量数据的分析,揭示了大气引力波的空间分布与极光椭圆的关系。在大量实验数据的基础上,建立了南极和北极上空波场的季节分布模式。对比分析了极地白天和极夜条件下两半球极地热层中AGWs的特征。根据kp指数,注意到agw分布的一些差异。观测到的AGW分布的季节特征及其对地磁活动水平的依赖性与太阳光照条件和地磁条件变化时极地风环流的重构有关。
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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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