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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Correlation between the ionospheric WN4 signature and the upper atmospheric DE3 tide
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Correlation between the ionospheric WN4 signature and the upper atmospheric DE3 tide

机译:电离层WN4签名之间的相关性和上层大气DE3潮流

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The present work studies the correlation relationship between the longitudinal ionospheric structure of wave number 4 (WN4) and the upper atmospheric tide of nonmigrating tidal mode DE3 (diurnal eastward wave number 3). Global ionospheric maps produced by the Jet Propulsion Laboratory were used to deduce the latitudinal integration of total electron content in the low-latitude ionosphere, and TIDI/TIMED observations were used to retrieve the atmospheric zonal and meridional winds. By applying Fourier filtering and fitting techniques, the WN4 wave and DE3 tidal components are derived from the ionospheric and upper atmospheric observations, respectively. We found that the observed WN4 wave and DE3 zonal wind components experience very similar annual and interannual variations, but the DE3 meridional wind component behaves in a quite different manner. Both WN4 and DE3 zonal winds are very intense during northern summer and autumn; they also appear in the later spring, but tend to vanish in winter. Their amplitudes increase as the solar activity decreases, and both are stronger in the quasi-biennial oscillation (QBO) eastward wind phase than in the westward phase. At the same time, the DE3 meridional wind likes to occur only in winter and seems not change with solar activity and QBO phase. We further studied the correlation between the WN4 wave and the two wind components of the DE3 tide. We found that the cross-correlation coefficient between the WN4 wave and the DE3 zonal wind is much larger, while that between the WN4 wave and the DE3 meridional wind is relatively smaller. Such different correlations are attributed to the different latitudinal symmetry of different DE3 wind components. The DE3 zonal wind is likely in latitudinally symmetric tidal mode; hence, it can efficiently affect the F region ion drifts. In contrast, the meridional wind is mainly in antisymmetric mode and thus seldom affects the ionospheric drifts. The present results support the suggestion that the longitudinal WN4 structure in the ionospheric F region originates from the symmetric modes, mainly the zonal wind component, of the upper atmospheric nonmigrating tidal mode DE3 in the ionospheric E region.
机译:目前的相关研究工作纵向电离层之间的关系波数4 (WN4)和结构上大气潮nonmigrating DE3潮汐模式(日东波数3)。全球电离层地图由喷气推进实验室被用来推导出纬度集成的总电子含量低纬度电离层,和TIDI /时间观察被用来检索大气纬向和经向风。应用傅里叶滤波和配件技术,WN4波和DE3潮汐组件来源于电离层和上吗分别大气观测。观察WN4波和DE3纬向风组件的经验和年度计划非常相似年际变化,但DE3子午风在不同组件的行为的方式。在北部夏季和秋季强烈;也出现在后来的春天,但往往在冬天消失。太阳活动减少,两者都是更强的quasi-biennial振荡(QBO)比西向东风阶段阶段。同时,DE3经向风喜欢只出现在冬季,似乎没有改变太阳活动和QBO的阶段。WN4波,两人之间的相关性风DE3潮流的组件。WN4之间的互关联系数波和DE3纬向风更大,, WN4波和DE3子午风是相对较小的。相关性是归因于不同的纬向对称不同DE3风组件。纬向对称的潮汐模式;有效地影响F离子漂移。相反,主要在经向风反对称模式,因此很少影响电离层的雪堆。纵向WN4的建议结构来源于电离层F地区从对称模式,主要是纬向风组件,上层大气nonmigrating潮汐模式DE3在电离层E地区。

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