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首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Vertical propagating signatures of wave-type oscillations (2- and 6.5-days) in the ionosphere obtained from electron-density profiles
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Vertical propagating signatures of wave-type oscillations (2- and 6.5-days) in the ionosphere obtained from electron-density profiles

机译:从电子密度剖面获得的电离层中波型振荡(2天和6.5天)的垂直传播特征

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摘要

We investigate the meteorology of wave-type oscillations in the period range of 2- and 6.5-days observed in the middle latitude ionosphere at the altitude range from 170 to 230 km during 1998, with an emphasis on their vertical propagation characteristics. The true height electron density profiles obtained at the Observatori de l'Ebre station (40.8°N, 0.5°E) have been used for this purpose. We found several events with occurrence of wave packets with periods near 2- and 6.5-days during the summer half-year. These events display a clear vertical progression in the ionospheric F region, with vertical wavelengths larger than 100 km. The events exist with upward or downward propagation and the different values between the phase and group velocities indicate the degree of dispersion that the ionosphere introduces on their propagation. The potential mechanisms linking the planetary wave activity in the mesosphere/lower thermosphere with the wave events observed in the ionosphere are discussed in order to evaluate the most likely mechanism.
机译:我们调查了1998年在中纬度电离层170至230 km高度范围内观测到的2天和6.5天周期范围内的波型振荡的气象,重点是它们的垂直传播特征。为此,使用了在埃伯雷观测站(40.8°N,0.5°E)获得的真实高度电子密度分布。我们在夏季半年中发现了几起与波包发生有关的事件,其周期分别为2天和6.5天。这些事件在电离层F区域显示出明显的垂直进展,垂直波长大于100 km。这些事件随着向上或向下传播而存在,并且相速度和群速度之间的不同值指示电离层在其传播过程中引入的分散程度。为了评估最可能的机理,讨论了将中层/下部热层中的行星波活动与电离层中观测到的波事件联系起来的潜在机理。

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