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Fresnel Zone and reflectarray antennas for space missions: Concepts, computational techniques and characterizations.

机译:太空任务的菲涅耳带和反射阵列天线:概念,计算技术和特征。

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Reflector antennas generally employ parabolic shaped main reflectors and have found a wide range of applications for both earth stations and satellite systems. Increasingly, one may find many advantages in minimizing antenna shaping requirement and weight as well as more compact designs by employing flat reflectors (either on the main reflector or on the subreflector) which can achieve a desired set of criteria for antenna performance. Two electrically large antennas which use flat min reflectors are Fresnel Zone (FZ) and reflectarray antennas which are being addressed in this dissertation. Analytical techniques are proposed, implemented, and verified to analyze these reflector geometries. A two dimensional (2-D) multi-scatterer analysis is formulated and implemented using various electromagnetic scattering techniques such as Physical Optics (PO), Method of Moments (MoM), and Geometrical Theory of Diffraction (GTD). The capability of the 2-D technique is further extended for dual reflector analysis with flat subreflector panels as well as design and analysis of FZ antennas with a proposed space missions application in solar sailing. FZ antenna design is based on establishing regions of quasi-uniform phases according to the PO current on the reflector face. The concepts extracted from the 2-D analysis of FZ reflectors is carried to the three dimensional (3-D) cases and incorporated into a multi reflector code, which has been widely used in variety of reflector applications. Like FZ antennas, reflectarrays work according to a similar set of principals by achieving a uniform phase current on the flat reflectarray surface. Accordingly, an analytical methodology is proposed and implemented within the structure of the multi-reflector code to analyze and give design criteria for both single and dual reflectarray configurations. This technique is compared to measured results published for single reflectarrays and is investigated for near-field Gregorian reflectarrays with beam scanning capabilities.
机译:反射天线通常采用抛物线形主反射器,并且在地球站和卫星系统中都有广泛的应用。越来越多地,通过采用平面反射器(在主反射器或副反射器上)可以达到天线性能的一组理想标准,在最小化天线成形要求和重量以及更紧凑的设计方面会发现许多优点。两个使用平面最小反射器的大天线是菲涅耳区(FZ)和反射阵列天线,本文将对此进行讨论。提出,实施和验证了分析技术,以分析这些反射镜的几何形状。使用各种电磁散射技术(例如物理光学(PO),矩量法(MoM)和几何衍射理论(GTD))来制定和实施二维(2-D)多散射体分析。二维技术的功能进一步扩展,可用于具有平面子反射器面板的双反射器分析以及拟议中的太空任务在太阳航行中的应用,以及FZ天线的设计和分析。 FZ天线设计基于根据反射器表面上的PO电流建立准均匀相的区域。从FZ反射器的2-D分析中提取的概念被带到三维(3-D)情况下,并合并到多反射器代码中,该代码已广泛用于各种反射器应用中。像FZ天线一样,反射阵列通过在平坦的反射阵列表面上实现均匀的相电流,从而根据一组相似的原理工作。因此,在多反射器代码的结构内提出并实施了一种分析方法,以分析并给出用于单反射阵列配置和双反射阵列配置的设计标准。将该技术与发布的单个反射阵列的测量结果进行了比较,并研究了具有光束扫描功能的近场格里高里反射阵列。

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