An empirical sea clutter model for low grazing angles

V. Gregers-Hansen, R. Mital
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引用次数: 22

Abstract

The most fundamental characteristic of sea clutter, as used in radar performance evaluation, is its apparent reflectivity defined as σ° (m2/m2). The word apparent is used here as a reminder that any measurement of sea clutter reflectivity inevitably includes the effects of propagation close to the sea surface. Sea clutter reflectivity depends on many factors including sea state, wind velocity, grazing angle, polarization, and radar frequency. A comprehensive tabulation of measurements from around 60 sources were included in the 1991 edition of Nathanson's book [1] and this probably represents the most complete database of sea clutter reflectivity available. Also included in this book by Nathanson was a detailed description of an empirical sea clutter model proposed by Horst et. al. [2], the so-called Georgia Technical Institute (GTI) model. This model has found widespread acceptance in the radar community although its technical basis may be somewhat vague.
低掠掠角海杂波经验模型
海杂波最基本的特征是其视反射率(σ°(m2/m2)),用于雷达性能评估。这里使用“明显”一词是为了提醒人们,对海杂波反射率的任何测量都不可避免地包括在海面附近传播的影响。海杂波反射率取决于海况、风速、掠角、极化和雷达频率等因素。1991年版的Nathanson的书[1]中包含了大约60个来源的测量结果的综合表,这可能是目前最完整的海杂波反射率数据库。Nathanson在这本书中还详细描述了Horst等人[2]提出的经验海杂波模型,即所谓的佐治亚技术学院(Georgia Technical Institute, GTI)模型。该模型在雷达社区中得到了广泛的接受,尽管其技术基础可能有些模糊。
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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