A Beam De-Broadening Algorithm for Atmospheric Radar

K. Nishimura, M. Kohma, Kaoru Sato, Toru Sato
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Abstract

Measuring the variance of the velocity of atmosphere $\sigma _{turb}^2$, which is proportionally linked to the energy dissipation rate, is a common role given to MST radar. However, the spectral width $\sigma _{obs}^2$, which is directly observable with a radar, contains not only the contribution from turbulence itself but also some measurement biases. Among them, beam broadening $\sigma _{beam}^2$, which is the projected components of the mean wind velocity to the off-center sensitivity of the radar beam, is the major factor. A number of studies have been conducted to evaluate the beam broadening under an assumption that the antenna beam is conical and well defined by its beam width. However, this assumption is not applicable to nonstandard radar configurations that have distributed or asymmetric antenna array and thereby resulting asymmetric beampatterns. We present a comprehensive mathematical theory and practical algorithm to evaluate $\sigma _{beam}^2$ that is applicable to any antenna structure.
一种大气雷达波束去展宽算法
测量大气速度的方差$\ σ _{turb}^2$,它与能量耗散率成比例地联系在一起,是MST雷达的常见任务。然而,用雷达直接观测到的光谱宽度$\sigma _{obs}^2$不仅包含湍流本身的贡献,还包含一些测量偏差。其中波束展宽$\sigma _{beam}^2$为平均风速对雷达波束偏离中心灵敏度的投影分量,是主要影响因素。在假设天线波束为锥形且由波束宽度确定的情况下,已经进行了许多研究来评估波束展宽。然而,这种假设不适用于具有分布式或非对称天线阵列的非标准雷达配置,从而导致非对称波束方向图。我们提出了一个全面的数学理论和实用的算法来评估$\sigma _{beam}^2$,适用于任何天线结构。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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