首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Tidal features in the wintertime mesospheric temperature and neutral winds recorded at Resolute Bay, Canada (74.68 degrees N, 94.90 degrees W)
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Tidal features in the wintertime mesospheric temperature and neutral winds recorded at Resolute Bay, Canada (74.68 degrees N, 94.90 degrees W)

机译:加拿大坚毅湾记录的冬季中层温度和中性风的潮汐特征(北纬74.68度,西经94.90度)

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The mesospheric temperature and neutral winds have been monitored from the Early Polar Cap Observatory, in the northern high latitude (Resolute Bay; 74.68 degrees N, 94.90 degrees W), Canada by a Michelson interferometer (MI) from 1997 to 2001 and a Fabry-Perot interferometer (FPI) from 1998 to 1999, respectively. The MI observes the nightglow OH (3-1) bands to derive temperature and airglow emission rate of the upper mesosphere. The FPI instrument provides the neutral wind data. For this study, we analyzed multi-year data taken from the above site and performed spectral analysis to retrieve tidal wave information. From the Lomb-Scargle spectral analysis of the measured temperatures, we find significant tidal oscillations at 8, 12, and 24 h periods. On the other hand, variations in the neutral wind are dominated by the 12- and 24-h period waves. Because of their periods and persistence, the observed oscillations are most likely of tidal origin, i.e. s = 0 non-migrating tides, for the temperature, which are known to have their maximum amplitudes at the pole based on past observations. However, we cannot rule out the other tidal components may also contribute to the observed oscillations. For the winds, at least the observed 12-h oscillation could be a solar-migrating tide with zonal wave number 2; again there may be some small contribution from other tidal components. (c) 2006 Elsevier Ltd. All rights reserved.
机译:1997年至2001年,加拿大的迈克尔逊干涉仪(MI)和法布里(Fabry-)分别从加拿大北高纬度地区(Resolute Bay;北纬74.68度,北纬94.90度)的早期极地帽天文台监测了中层温度和中性风。佩罗干涉仪(FPI)分别从1998年到1999年。 MI观测夜光OH(3-1)波段,以推算上部中层大气的温度和气辉发射率。 FPI仪器提供中性风数据。对于本研究,我们分析了从上述站点获取的多年数据,并进行了频谱分析以检索潮汐信息。通过对测得温度的Lomb-Scargle光谱分析,我们发现在8、12和24 h周期内出现明显的潮汐振荡。另一方面,中性风的变化主要由12小时和24小时周期波控制。由于它们的周期和持续性,所观测到的振荡很可能是潮汐起源的,即对于温度而言s = 0非迁移潮汐,根据过去的观测已知在极点具有最大振幅。但是,我们不能排除其他潮汐分量也可能导致观测到的振荡。对于风来说,至少观察到的12小时振荡可能是纬向波数为2的太阳迁移潮。同样,其他潮汐成分可能也有一些贡献。 (c)2006 Elsevier Ltd.保留所有权利。

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