在归一化站点衰减测量中使用小型双锥天线的评估

Hironari Tanaka, Ikuo Makino, H. Shimanoe, H. Muramatsu
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引用次数: 3

摘要

辐射发射测量站点的验证通常通过使用宽带天线在30 MHz至1 GHz范围内进行归一化站点衰减(NSA)测量来执行,如ANSI 63.4和CISPR 16-1-4等标准所建立的那样。在标准方法中,通常使用30mhz至200mhz范围内的双锥天线和200mhz至1ghz范围内的对数周期偶极子天线。同时,我们看到在整个频率范围内使用小型双锥天线进行NSA测量的情况,因此,我们VCCI决定进行一系列实验,以评估在NSA测量中使用小型双锥天线的可行性,并与典型的Bicon/LPD天线进行对比。在一系列实验之前,我们进行了NSA天线因子校准,发现小型双锥天线由于天线因子较大,需要NSA测量系统能够确保140dB或更高的宽动态范围。实验了各天线的天线阻抗和辐射方向图的差异。本评估中的NSA测量是在每个天线的三个3米sac和两个10米sac进行的。结果发现,虽然在200 MHz以下与标准方法差异不大,但在200 MHz以上由于天线辐射方向图的差异而差异明显,在500 MHz以上由于天线杆反射的影响而差异明显。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
An evaluation of using small biconical antennas in normalized site attenuation measurements
Validation of radiated emission measurement sites is usually performed through normalized site attenuation (NSA) measurements in 30 MHz to 1 GHz using broadband antennas, as established in such standards as ANSI 63.4 and CISPR 16-1-4. By the standard method, it is typical to use a biconical antenna in the 30 MHz to 200 MHz range and a log-periodic dipole antenna in the 200 MHz to 1 GHz range. Meanwhile, we see cases of using a small biconical antenna in NSA measurements over the entire frequency range Therefore, we, VCCI decided to conduct a series of experiments to evaluate the feasibility of using small biconical antennas in NSA measurements, as contrasted to typical Bicon/LPD antennas. Prior to a series of experiments, we conducted NSA antenna factor calibration, and found small biconical antennas would require an NSA measuring system being able to ensure a wide dynamic range of 140dB or more due to their large antenna factors. Also we experimented the differences of antenna impedance and radiation patterns of each antenna. NSA measurements in this evaluation were conducted at three 3 m SACs and twe 10 m SACs of each antenna. As the results, we found that, although there were little differences from the standard method below 200 MHz, differences were apparent above 200 MHz by the difference of antenna radiation patterns and above 500 MHz by the effect of reflections from the antenna mast.
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