首页> 外文期刊>Radio Science >Observations of mesospheric wind velocities, 2. Cross sections of power spectral density for 48-8 hours, 8-1 hours, and 1 hour to 10 min over 60-110 km for 1981
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Observations of mesospheric wind velocities, 2. Cross sections of power spectral density for 48-8 hours, 8-1 hours, and 1 hour to 10 min over 60-110 km for 1981

机译:中空风速的观测; 1981年60-110 km上48-8小时,8-1小时和1小时至10分钟的功率谱密度横截面

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Cross sections of power spectral density for 1981 between 60-110 km for the 48- to 8 hour- and 8- to 1-hour-period bands, and of mean square velocity components in the 10- to 60-min-period band, are compared to cross sections of mean wind. Individual spectra agree well in form and amplitude to similar spectra for other sites when averaged over the entire year, but there are substantial variations in power spectral density in each band over the year. In the 10-min to 8-hour-period band, minima in spectral densities follow the zero line of mean zonal velocity very closely, indicating strong gravity wave mean flow interactions. This, and the variation in gravity wave intensity in general, suggests that gravity wave momentum deposition plays an important role in balancing the heat and momentum budgets of the upper middle atmosphere.
机译:1981年功率谱密度的横截面,介于48至8小时和8至1小时时段的60-110 km之间,以及10至60分钟时段的均方速度分量,与平均风的横截面进行比较。全年平均后,各个频谱的形式和幅度与其他站点的类似频谱非常吻合,但是一年中每个频段的功率频谱密度存在很大差异。在10分钟到8小时的频带中,光谱密度的最小值非常接近平均纬向速度的零线,表明强烈的重力波平均流相互作用。这以及重力波强度的一般变化表明,重力波动量沉积在平衡中高层大气的热量和动量预算方面起着重要作用。

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