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Experimental investigation of the dynamics near the winter northern polar mesopause.

机译:冬季北半球中游附近动力学的实验研究。

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摘要

An investigation of the dynamics near the winter northern polar mesopause has been carried out at the Early Polar Cap Observatory at Resolute Bay, Canada (74.9°N, 94.9°W). Tidal and planetary wave characteristics were studied using experimental and theoretical tools. The daily, monthly, and annual variations of the tidal field were studied using the 1995/1996 and 1996/1997 data. Ground-based measurements were obtained using a Fabry-Perot Interferometer with a Circle-to-Line Interferometric Optical system (FPI/CLIO) and an E-Region Wind Interferometer (ERWIN). The FPI/CLIO observed the Doppler winds of the OH emission near 86 km. The ERWIN provided simultaneous OH (86 km) and O1S (97 km) wind measurements. Monthly data were compared to the Global Scale Wave Model (GSWM) and the Forbes/Vial Solar Semidiurnal Tidal Model predictions. Additionally, a Global Empirical Vector Spherical Harmonics (VSH) Model was used to investigate the seasonal upper mesosphere and lower thermosphere tides.; Classical tidal theory predicts that the winter polar region is relatively undisturbed by tides---oscillations of integral sub-harmonics of one day. Contrary to this theory, the semidiurnal (12 h) oscillation has been detected at Resolute. Analysis of this oscillation at 86 and 97 km, indicates that it is persistent and characteristic of a semidiurnal propagating tide. The research presented constitutes the first long-term study (∼3 months of data over 2 years) of the dynamical structure of the winter northern polar mesopause using optical instruments. Significant and new contributions include that the semidiurnal tide has been found to be highly variable in amplitude and phase from day to day. Planetary waves with periods near 5, 8, and 16 d are shown to modulate the semidiurnal amplitudes and background winds. In addition, non-linear interactions between planetary waves and the semidiurnal tide are detected near the polar mesopause. Spectral analysis reveal a variety of waves---tidal waves, planetary waves, and secondary waves as a result of non-linear wave interactions---which are geophysical and not attributed to spectral leakage.
机译:在加拿大坚毅湾(74.9°N,94.9°W)的极地极顶天文台进行了冬季北极中层顶附近动力的调查。使用实验和理论工具研究了潮汐和行星波的特征。使用1995/1996和1996/1997数据研究了潮汐场的每日,每月和每年变化。地面测量是使用具有圆到线干涉光学系统(FPI / CLIO)和E-区域风干涉仪(ERWIN)的Fabry-Perot干涉仪获得的。 FPI / CLIO观察到OH发射的多普勒风接近86 km。 ERWIN可以同时进行OH(86公里)和O1S(97公里)风的测量。将月度数据与全球尺度波浪模型(GSWM)和《福布斯/小太阳日半潮汐模型》的预测进行了比较。此外,还使用了一个全球经验矢量球谐函数(VSH)模型来调查季节性中高层和较低热层潮汐。古典潮汐理论预测,冬季极地地区相对不受潮汐的干扰,即一天中整体次谐波的振荡。与该理论相反,在Resolute处检测到半日振荡(12小时)。对这种在86 km和97 km处的振荡的分析表明,它是持续存在的,并且是半日增潮的特征。提出的研究是使用光学仪器对冬季北极极中年期动力学结构进行的首次长期研究(约2个月的3个月数据)。重要的和新的贡献包括发现半日潮在每天的振幅和相位上变化很大。图中显示了周期约为5、8和16 d的行星波调制半日振幅和背景风。此外,在极地中生极附近发现了行星波与半日潮之间的非线性相互作用。频谱分析揭示了各种波-非线性波相互作用导致的潮汐波,行星波和次级波-是地球物理波,而不是归因于频谱泄漏。

著录项

  • 作者

    Fisher, Genene Michelle.;

  • 作者单位

    University of Michigan.;

  • 授予单位 University of Michigan.;
  • 学科 Physics Atmospheric Science.
  • 学位 Ph.D.
  • 年度 2001
  • 页码 192 p.
  • 总页数 192
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 大气科学(气象学);
  • 关键词

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