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Feasibility study of a novel class of plasma antennas for SatCom navigation systems

机译:SATCOM导航系统新型等离子体天线的可行性研究

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Gaseous Plasma Antennas (GPAs) are devices that exploit weakly or fully ionized gases to transmit and receive electromagnetic (EM) waves. GPAs can offer several advantages over their metallic counterparts since radiation pattern, gain and operating frequency depend on the electrical response of the plasma. A particularly appealing field in which these antennas could be exploited is the Global Navigation Satellite System (GNSS). In fact, GPAs allow to meet the increasingly strict requirements imposed on the GNSS application; specifically, they can drastically reduce multipath errors. This feature is particularly important for the future use of GNSS in critical networks, as for example Public Protection and Disaster Relief (PPDR). In order to verify whether GPAs can be realistically exploited on this field, a preliminary analysis has been accomplished to assess their performances in the L band (i.e., the frequency range proper of GNSS operations). Specifically, two circularly polarized antennas, conceived as the basic elements of an array of GPAs, have been compared. The two concepts, namely a curl and a turnstile antenna, have been characterized in terms of reflection coefficient, axial ratio, and maximum gain. A combined numerical and experimental approach has been adopted for this analysis. Dedicated plasma sources have been manufactured in-house to obtain a realistic evaluation of the plasma parameters. Specifically, the plasma density and the background neutral pressure have been measured with a Pirani gauge and a microwave interferometer, respectively. Once these parameters are known, and in turn the electrical response of the plasma has been assessed, the characteristics of the two antennas have been numerically calculated by means of the commercial software CST Microwave Studio (R). The curl antenna concept results the most promising one provided that it satisfies the functional requirements imposed by GNSS application (i.e., circular polarization in the L-frequency band).
机译:气体等离子体天线(GPA)是利用弱或完全电离气体来传输和接收电磁(EM)波的装置。由于辐射图案,增益和工作频率取决于等离子体的电响应,GPA可以提供几个优于金属对应物的优点。可以利用这些天线的特别有吸引力的领域是全球导航卫星系统(GNSS)。事实上,GPA允许满足GNSS申请越来越严格的要求;具体来说,它们可以急剧减少多径错误。此功能对于未来在关键网络中使用GNSS尤其重要,例如公共保护和救灾(PPDR)。为了验证GPA是否可以在该领域进行实际利用,已经完成了初步分析以评估L频带中的性能(即,GNSS操作的频率范围)。具体地,已经比较了两个被认为是作为GPA阵列的基本元素的圆偏振天线。两个概念,即卷曲和旋转天线,已经表征了反射系数,轴向比和最大增益。该分析采用了组合的数值和实验方法。专用的等离子体来源已经在内部制造,以获得对等离子体参数的实际评估。具体地,分别用Pirani表和微波干涉仪测量等离子体密度和背景中性压力。一旦这些参数是已知的,并且反过来已经评估了等离子体的电响应,通过商业软件CST微波演播室(R),已经用商业软件进行了数量计算了两种天线的特性。卷曲天线概念结果是最有希望的,提供了它满足GNSS应用(即L频带中的圆极化)施加的功能要求。

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