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Tidal wind oscillations in the tropical lower atmosphere as observed by Indian MST Radar

机译:印度MST雷达观测到的热带低层大气中的潮汐风振荡

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摘要

Diurnal tidal components in horizontal winds measured by MST radar in the troposphere and lower stratosphere over a tropical station Gadanki (13.5° N, 79.2° E) are presented for the autumn equinox, winter, vernal equinox and summer seasons. For this purpose radar data obtained over many diurnal cycles from September 1995 to August 1996 are used. The results obtained show that although the seasonal variation of the diurnal tidal amplitudes in zonal and meridional winds is not strong, vertical phase propagation characteristics show significant seasonal variation. An attempt is made to simulate the diurnal tidal amplitudes and phases in the lower atmosphere over Gadanki using classical tidal theory by incorporating diurnal heat sources, namely, solar radiation absorption by water vapour, planetary boundary layer (PBL) heat flux, latent heat release in deep convective clouds and short wave solar radiation absorption by clouds. A comparison of the simulated amplitudes and phases with the observed ones shows that agreement between the two is quite good for the equinox seasons, especially the vertical structure of the phases of the meridional wind components.Key words. Meteorology and atmospheric dynamics (tropical meteorology; waves and tides)
机译:由MST雷达在热带站Gadanki(13.5°N,79.2°E)的对流层和低平流层中测量的水平风的昼夜潮汐分量介绍了秋分,冬季,春分和夏季的季节。为此,使用了从1995年9月到1996年8月的许多日周期中获得的雷达数据。获得的结果表明,尽管纬向和经向风的日潮幅值的季节变化并不强烈,但垂直相位传播特征却显示出明显的季节变化。通过经典的潮汐理论,尝试通过结合昼夜热源,即水蒸气吸收的太阳辐射,行星边界层(PBL)热通量,潜热释放,深对流云和短波太阳辐射被云吸收。将模拟的振幅和相位与观测到的振幅和相位进行比较表明,在春分季节,两者之间的一致性非常好,尤其是子午风分量相位的垂直结构。 关键词。 气象和大气动力学(热带气象;海浪和潮汐)

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