1.25GHz相控阵馈电的阵列设计

Hao Yan, Kai Wang, Liang Cao, Mao-zheng Chen, Jun Ma, X. Duan
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引用次数: 1

摘要

相控阵馈电是一种能够使射电望远镜实现连续视场覆盖的接收技术。结合反射面天线的特点,通过各种设计下的焦场分析和性能比较,提出了1.25 GHz相控阵馈电的具体阵列设计方法。最终设计的相控阵馈电在1.25 GHz工作频率下可实现3倍于望远镜视场的波束宽度,阵列尺寸为0.525m,阵元间距为波长的0.437倍,阵列排列方式为六角形排列,最终阵元数为19个,其中7个阵元的六角形子阵形成1束。虽然上述阵列设计参数不是相同条件下的最优解,但相关步骤可以指导反射面天线相控阵馈电的阵列设计,也为后期宽带和超宽带相控阵馈电阵列的设计提供参考。
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Array Design of Phased Array Feed at 1.25GHz
Phased array feed is a receiver technology that can make the radio telescope achieve continuous field of view coverage. Combined with the characteristics of reflector antenna, through focal field analysis and performance comparison under various designs, this paper presents the specific array design method of 1.25 GHz phased array feed. The final designed phased array feed can achieve three times the beam width of the telescope field of view at the working frequency of 1.25 GHz, the array size is 0.525m, the array element spacing is 0.437 times the wavelength, the array arrangement mode is hexagonal arrangement, and the final number of array elements is nineteen, of which the hexagonal subarray of 7 elements form one beam. Although the above array design parameters are not the optimal solution under the same conditions, the relevant steps can guide the array design of reflector antenna phased array feed, and also provide a reference for the later design of broadband and ultra wideband phased array feed array.
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