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Numerical modeling of the solar and lunar semidiurnal atmospheric tides has been performed by invoking a comprehensive approach that includes both algebraic manipulation and numerical solution of the primitive equation system. The effect of latitudinally varying temperature and associated mean zonal wind in a modeled atmosphere with realistic forcing are successfully incorporated to reproduce tidal variabilities at meteor heights delineated by varieties of radar observations.
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Asô et al. (1981) studied this question.
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