一种新型电子可重构X/Ku波段反射天线的优化设计

V. Suresh
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引用次数: 1

摘要

本文报道的频率可重构反射射线(RRA)提供了三个频率的铅笔波束,满足了卫星广播电视在Ku波段和X波段上行和下行频率上的需求。为了实现这种频率重构,基于无限阵列方法开发和模拟的单元格与四个PIN二极管集成使用,分别在14.34 GHz上行、12.2 GHz下行和11.9 GHz x波段性能下产生525°、415°和308°的反射相位变化。在该单元中,上行链路的相位变化是通过改变同心环的大小来实现的,而在下行链路和x波段的情况下,由引脚二极管控制的重构是通过改变延迟线的长度来实现的。利用所设计的单元格,在平面正方形几何结构上构造了一个包含225个单元的15 - 15阵列,周期为0.49λ0 (10.5 mm)。在14.34 GHz、12.2 GHz和11.9 GHz时,最大增益分别为25.77 dBi、25.13 dBi和22.7 dBi,孔径效率分别为40.22%、26.46%和25.36%。仿真结果表明,三种工作频率下-3dB增益带宽分别为8.37%、4.92%和12.18%。因此,这种可重构反射天线在深空通信和直接广播卫星应用中可作为抛物面反射器和相控阵天线的仿真替代品,满足高增益铅笔波束的要求。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Optimum Design of a Novel Electronically Reconfigurable Reflectarray Antenna for X/Ku Band Applications
The frequency reconfigurable reflectarray (RRA) reported in this paper provides a pencil beam at three frequencies captivating the need for satellite broadcast television at uplink and downlink frequencies in Ku band and X band. To achieve such frequency reconfiguration, a unit cell developed and simulated based on an infinite array approach is used in integration with four PIN diodes to produce a reflection phase variation of 525°, 415°, and 308° at 14.34 GHz for uplink operation, 12.2 GHz for downlink and 11.9 GHz for X-band performance respectively. In this proposed unit cell, the phase variation for uplink is achieved by varying the size of concentric loops, while in the case of downlink and X-band, reconfiguration controlled by pin diodes is achieved by varying the length of the delay line. With the periodicity of 0.49λ0 (10.5 mm), a 15 15 array with 225 elements is constructed using the designed unit cell on square planar geometry. The paper reports a maximum gain of 25.77 dBi, 25.13 dBi, and 22.7 dBi and 40.22%, 26.46%, and 25.36% of aperture efficiency at 14.34 GHz, 12.2 GHz, and 11.9 GHz respectively. A -3dB gain bandwidth of 8.37%, 4.92%, and 12.18% is achieved at the three operating frequencies by simulation. Hence this reconfigurable reflectarray serves as an emulous alternative to parabolic reflectors and phased array antennas in deep space communication and direct broadcast satellite applications satisfying the high gain pencil beam requirements.
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