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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Troposphere-thermosphere tidal coupling as measured by the SABER instrument on TIMED during July–September 2002
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Troposphere-thermosphere tidal coupling as measured by the SABER instrument on TIMED during July–September 2002

机译:Troposphere-thermosphere潮汐耦合,军刀仪器测量的时间2002年7月- 9月

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Coupling between the troposphere and lower thermosphere due to upward propagating tides is investigated using temperatures measured from the SABER instrument on the TIMED satellite. The data analyzed here are confined to 20–120 km altitude and ±40° latitude during 20 July to 20 September 2002. Apart from the migrating (Sun-synchronous) tidal components, the predominant feature seen (from the satellite frame) during this period is a wave-4 structure in longitude with extrema of up to ±40–50 K at 110 km. Amplitudes and longitudes of maxima of this structure evolve as the satellite precesses in local time and as the wave(s) responsible for this structure vary with time. The primary wave responsible for the wave-4 pattern is the eastward propagating diurnal tide with zonal wave number s = 3 (DE3). Its average amplitude distribution over the interval is quasi-symmetric about the equator, similar to that of a Kelvin wave, with maximum of about 20 K at 5°S and 110 km. DE3 is primarily excited by latent heating due to deep tropical convection in the troposphere. It is demonstrated that existence of DE3 is intimately connected with the predominant wave-4 longitude distribution of topography and land-sea difference at low latitudes, and an analogy is drawn with the strong presence of DE1 in Mars atmosphere, the predominant wave-2 topography on Mars, and the wave-2 patterns that dominate density measurements from the Mars Global Surveyor (MGS) spacecraft near 130 km. Additional diurnal, semidiurnal, and terdiurnal nonmigrating tides are also revealed in the present study. These tidal components are most likely excited by nonlinear interactions between their migrating counterparts and the stationary planetary wave with s = 1 known to exist in the Southern Hemisphere during this period just prior to the austral midwinter stratospheric warming of 2002.
机译:对流层和低之间的耦合热电离层由于向上传播的潮汐使用温度测量的研究军刀的卫星仪器。分析下面是局限于20 - 120公里的高度和40°±7月20日至9月20日期间纬度2002. 潮汐组件,主要特性在此期间(从卫星帧)wave-4结构与极值的经度在110公里到±40 - 50 K。经度最大值的结构演变卫星绕着在当地时间波(s)负责这个结构随时间。模式是向东传播全日潮纬向波数s = 3 (DE3)。振幅分布区间quasi-symmetric赤道,类似开尔文波的,最大的约20 K在5°和110公里。潜在的因深热带对流加热对流层。存在DE3是紧密相连的主要wave-4经度分布在低近年地形和区别纬度,类比的火星大气中存在DE1强,火星上的主要wave-2地形,wave-2模式主导密度从火星环球探测器测量(毫克)宇宙飞船接近130公里。半日,terdiurnal nonmigrating潮汐在目前的研究还揭示了。潮汐组件是最有可能兴奋不已迁移之间的非线性相互作用同行和静止的行星波和s = 1存在于南方在此期间半球前南国冬至2002年平流层变暖。

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