阵列变形性能对低轨l波段GMTI SBR的影响

P. Zulch, R. Hancock, J. Mckay
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引用次数: 7

摘要

天基雷达(SBR)已经研究了几十年,并再次作为执行运动目标指示(MTI)任务的可行方法出现。这种应用需要大型阵列,以便在目标上提供足够的能量进行探测,并尽量减少观测到的地杂波多普勒传播。空间中的大型相控阵很可能在子阵面板水平和整个结构上经历机械变形。分析了天线变形对天线方向图、峰值定向增益和信噪比损耗(SINRL)的影响,并对最小可识别速度(MDV)产生影响。本文讨论了应用于美国空军(USAF)和NASA感兴趣的基于低地球轨道(LEO)的l波段雷达概念时的变形
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Array deformation performance impacts on a LEO L-band GMTI SBR
Space based radar (SBR) has been investigated for decades and has once again made an appearance as a viable method for performing the moving target indication (MTI) mission. Large arrays are needed for this application in order to provide adequate energy on target for detection and to minimize the observed ground clutter Doppler spread. Large phased arrays in space are likely to experience mechanical deformation both at the sub-array panel level and across the structure as a whole. The impact of antenna deformations on antenna pattern, peak directive gain, and signal to interference plus noise ratio loss (SINRL), which shows impact on minimum discernable velocity (MDV), is demonstrated. This paper address the deformations when applied to a low earth orbit (LEO) based L-band radar concept of interest to the US Air Force (USAF) and NASA
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