利用合成探针阵列技术测量室内反射环境中的低频天线

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

摘要

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