Measurement of Low Frequency Antennas in Indoor Reflective Environments with the Synthetic Probe Array Technique

R. T. Sánchez, F. Saccardi, A. Giacomini, M. Saporetti, P. Moseley, L. Foged
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引用次数: 4

Abstract

Performance verification of low gain antennas on small space platforms are challenging at frequencies below 400MHz, also owing to limitations in the anechoic environment. Spherical near-field measurement techniques are often applied in such cases, enabling different echo-reduction schemes to compensate for the non-ideal test environment. Uncertainties due to chamber reflections are also reduced with a directive probe but electrically larger probes are impractical at very low frequencies because of the resulting physical dimensions. A virtual probe, synthesized from an array of smaller probes, with limited wall illumination has been developed to reduce this error. The concept has been developed for measurements in the ESA/ESTEC HERTZ testing facility of the HERA-JUVENTAS mission with a 50–70 MHz dipole antenna mounted on a CubeSat. In this paper, we present the concept, feasibility, and verification by measurements on a 10:1 scaled representation of the CubeSat scenario and the HERTZ facility.
利用合成探针阵列技术测量室内反射环境中的低频天线
由于消声环境的限制,在低于400MHz的频率下,小空间平台上的低增益天线的性能验证具有挑战性。球面近场测量技术通常应用于这种情况,使不同的回波减少方案,以补偿非理想的测试环境。由于腔室反射的不确定性也减少了指示探头,但由于产生的物理尺寸,电较大的探头在非常低的频率下是不切实际的。一种虚拟探针,由一组较小的探针合成,具有有限的墙壁照明,以减少这种误差。这个概念是为了在HERA-JUVENTAS任务的欧空局/ESTEC赫兹测试设施中进行测量而发展起来的,该设施安装在一颗立方体卫星上的50-70兆赫偶极子天线。在本文中,我们提出了概念、可行性,并通过测量CubeSat场景和HERTZ设施的10:1比例表示进行了验证。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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