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1.2 Meter Shielded Cassegrain Antenna for Close-Packed Radio Interferometer

机译:用于封闭收音机的1.2米屏蔽卡塞格伦天线   干涉仪

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摘要

Interferometric millimeter observations of the cosmic microwave backgroundand clusters of galaxies with arcmin resolutions require antenna arrays withshort spacings. Having all antennas co-mounted on a single steerable platformsets limits to the overall weight. A 25 kg lightweight novel carbon-fiberdesign for a 1.2 m diameter Cassegrain antenna is presented. The finite elementanalysis predicts excellent structural behavior under gravity, wind and thermalload. The primary and secondary mirror surfaces are aluminum coated with a thinTiO$_2$ top layer for protection. A low beam sidelobe level is achieved with aGaussian feed illumination pattern with edge taper, designed based on feedhornantenna simulations and verified in a far field beam pattern measurement. Ashielding baffle reduces inter-antenna coupling to below $\sim$ -135 dB. Theoverall antenna efficiency, including a series of efficiency factors, isestimated to be around 60%, with major losses coming from the feed spilloverand secondary blocking. With this new antenna, a detection rate of about 50clusters per year is anticipated in a 13-element array operation.
机译:对宇宙微波背景和具有arcmin分辨率的星系团进行干涉式毫米波观测需要天线阵列具有较短的间距。将所有天线共同安装在单个可操纵平台上会限制整体重量。提出了一种25千克轻巧的新型碳纤维设计,用于直径为1.2 m的卡塞格伦天线。有限元分析预测在重力,风和热负荷下的优异结构行为。主镜和副镜表面均镀有铝,上面涂有一层薄的TiO $ _2 $以进行保护。低光束旁瓣电平是通过具有高锥度的高斯馈电照明图案实现的,该图案是基于馈电喇叭天线仿真设计的,并在远场光束图案测量中得到了验证。屏蔽挡板将天线之间的耦合降低到$ \ sim $ -135 dB以下。包括一系列效率因素在内的总体天线效率估计约为60%,主要损失来自馈电溢出和二次阻塞。使用这种新天线,预计在13个元素的阵列操作中,每年的检测率约为50个簇。

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