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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:由SABER仪器在2002年7月至9月间对TIMED进行的对流层-热层潮汐耦合

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摘要

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:使用从定时卫星上的SABER仪器测得的温度,研究了由于潮汐向上传播而导致的对流层和较低热层之间的耦合。在2002年7月20日至9月20日期间,此处分析的数据仅限于20-120 km的高度和±40°的纬度。除了正在迁移的(与太阳同步)潮汐分量外,在此期间(从卫星帧)看到的主要特征是经波4结构,在110 km处极值可达±40–50K。这种结构的最大值的振幅和经度随着卫星进动在当地时间和负责这种结构的波随时间变化而变化。负责第4波模式的主要波是向东传播的昼夜潮,其纬向波数s = 3(DE3)。其在整个区间内的平均幅度分布关于赤道是准对称的,类似于开尔文波,在5°S和110 km处的最大值约为20K。由于对流层中的热带深对流作用,DE3主要由潜在的加热激发。结果表明,DE3的存在与地形的优势波4经度分布和低纬度海陆差异密切相关,并以DE1在火星大气中的强烈存在作为类比,主导了优势波2地形。火星上的第二波模式和火星全球测量师(MGS)太空船在130公里附近的密度测量中占主导地位的第二波模式。在本研究中还发现了其他的日,半日和日非潮汐潮汐。这些潮汐分量最有可能是由它们的迁移对应物与s = 1的固定行星波之间的非线性相互作用激发的,该行星波在2002年南半球平流层冬季变暖之前的那个时期存在于南半球。

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