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Radar estimations of atmospheric winds in the troposphere and lower stratosphere.

机译:对流层和低平流层中大气风的雷达估计。

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摘要

This dissertation deals with the estimation of atmospheric flow field parameters using the spaced antenna (SA) and spatial interferometer (SI) methods. In the first section, a computer simulation of scattering from inhomogeneities in the refractive index is used to compare the SA and SI methods for measuring winds in clear air both with and without turbulent fading. The results show that the SA analysis which is carried out in the time domain and the SI analysis which is carried out in the frequency domain are equivalent in terms of the information that the two methods yield. A data analysis method equivalent to full correlation analysis, which can be carried out in the frequency domain, is presented. The method is applied to model-generated data in order to extract the typical full correlation analysis output parameters such as the apparent and true velocities. The results obtained are consistent with the model input parameters. In the second section a statistical comparison of the SA and SI methods for estimating horizontal winds in the troposphere and the lower stratosphere is presented. The data analyzed were obtained with the Middle and Upper (MU) atmosphere radar from 1910 LT on June 29, 1990, through 0950 LT on July 2, 1990. At all heights, velocity estimates based on frequency domain data are within 4% of those based on time domain data. We conclude that frequency domain techniques provide an alternate method for estimating true horizontal velocity. Nevertheless, it is not clear that they offer any significant advantage over time domain methods. In fact, the results obtained indicate that the SI method for estimating horizontal velocity may be slightly more difficult to apply in practice. The final section presents an analytical evaluation of SA-based instrumental setups with the potential for estimating the vertical component of atmospheric vorticity from a single-radar location. Methods considered are the oblique spaced antenna (OAS) method and a modified SA system employing four vertically-pointed receiving antennas. Analogies are drawn between the Doppler and SA methods, and it is concluded that the two systems gather the same information when atmospheric turbulence is small and the reflectivity is uniform. Furthermore, it is concluded that under normal conditions measurement uncertainties will preclude the estimation of atmospheric vorticity from a single-radar location.
机译:本文采用空间天线(SA)和空间干涉仪(SI)方法对大气流场参数进行估计。在第一部分中,使用计算机模拟了折射率不均匀性引起的散射,以比较SA和SI方法在有或没有湍流衰落的情况下在清澈的空气中测量风的能力。结果表明,就两种方法产生的信息而言,在时域中进行的SA分析和在频域中进行的SI分析是等效的。提出了一种等效于全相关分析的数据分析方法,可以在频域中进行。该方法应用于模型生成的数据,以提取典型的全相关分析输出参数,例如视在和真实速度。获得的结果与模型输入参数一致。在第二部分中,对估计对流层和低平流层中水平风的SA和SI方法进行了统计比较。分析的数据是使用1990年6月29日的1910 LT和1990年7月2日的0950 LT的中高层(MU)大气雷达获得的。在所有高度上,基于频域数据的速度估计都在这些高度的4%以内基于时域数据。我们得出结论,频域技术提供了一种估计真实水平速度的替代方法。然而,尚不清楚它们是否比时域方法具有明显优势。实际上,获得的结果表明,用于估算水平速度的SI方法可能在实践中可能会稍微困难一些。最后一部分介绍了基于SA的仪器设置的分析评估,并具有从单雷达位置估算大气涡度垂直分量的潜力。所考虑的方法是倾斜间隔天线(OAS)方法和采用四个垂直指向的接收天线的改良SA系统。用多普勒和SA方法进行类比,得出结论,当大气湍流较小且反射率均匀时,这两个系统收集相同的信息。此外,得出的结论是,在正常条件下,测量不确定性将排除从单雷达位置估算大气涡度的可能性。

著录项

  • 作者

    Sheppard, Emory Lamar.;

  • 作者单位

    Clemson University.;

  • 授予单位 Clemson University.;
  • 学科 Physics Atmospheric Science.;Physics Fluid and Plasma.
  • 学位 Ph.D.
  • 年度 1992
  • 页码 88 p.
  • 总页数 88
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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