Long wave antenna design for CALLISTO System

Supun Liyanaarachchi, J. Adassuriya, K. Jayaratne
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Abstract

Life on the surface of the earth is highly affected by solar activities. The real time observations of these solar activities are highly important to minimize the effect on the earth system. Solar radio observations are relevant to the study of such phenomena. The Compound Astronomical Low-frequency Low-cost Instrument for Spectroscopy and Transportable Observatory (CALLISTO) system is one method to study the solar radio bursts. This paper highlights a new study leading to the development of a long wave antenna (LWA) design, which is proposed for a new CALLISTO station. Generally, the solar radio bursts are circularly polarized and more often observed in low regions of the high frequency (HF) and very high frequency (VHF) bands. Therefore, the antenna is designed for the frequency range of 20 MHz to 100 MHz. The designing of the antenna was done using 4nec2 software, a Numerical Electromagnetics Code (NEC) based antenna modeller and an optimizer. The main structure of the design contains two identical antennas in both north-south and east-west directions. The performance of the design was tested by changing the dimensions and simulating the model to optimize the parameters. Considerable performance increases could be observed by applying the ground plane to the antenna model. The resulting performance by simulation shows average gain test (AGT) values of 1.923 at 15 MHz, 2.001 at 30 MHz, 2.021 at 50 MHz, 2.056 at 70 MHz and 2.096 at 100 MHz. The 1.90 - 2.10 AGT range ensures the model is perfect with the input parameters for the physical production. The maximum gain was obtained as 9.12 dB at 50 MHz and in the frequency range considered, this design could maintain a gain higher than 7 dB. The other important performance factors, voltage standing wave ratio (VSWR), structure loss, efficiency, left-hand circular polarization (LHCP) and right-hand circular polarization (RHCP) gain, etc. are also observed. From the simulations, it was observed that LHCP gain is always dominating total gain.
CALLISTO系统的长波天线设计
地球表面的生命受太阳活动的影响很大。对这些太阳活动的实时观测对于最小化其对地球系统的影响是非常重要的。太阳射电观测与这类现象的研究有关。复合低频低成本光谱仪和可移动天文台(CALLISTO)系统是研究太阳射电暴的一种方法。本文重点介绍了一项新的研究,该研究导致了长波天线(LWA)设计的发展,该设计被提议用于一个新的CALLISTO站。一般来说,太阳射电暴是圆极化的,并且更经常在高频(HF)和甚高频(VHF)波段的低区域观测到。因此,天线设计的频率范围为20mhz ~ 100mhz。利用4nec2软件、基于数值电磁法(NEC)的天线建模器和优化器对天线进行了设计。设计的主要结构包括南北和东西方向的两个相同的天线。通过改变尺寸和模拟模型来优化参数,验证了设计的性能。通过将地平面应用于天线模型,可以观察到相当大的性能提高。仿真结果表明,平均增益测试(AGT)值在15 MHz时为1.923,在30 MHz时为2.001,在50 MHz时为2.021,在70 MHz时为2.056,在100 MHz时为2.096。1.90 - 2.10 AGT范围确保模型与物理生产的输入参数完美匹配。在50 MHz时获得的最大增益为9.12 dB,在考虑的频率范围内,本设计可以保持高于7 dB的增益。此外,还观察了电压驻波比(VSWR)、结构损耗、效率、左圆极化(LHCP)和右圆极化(RHCP)增益等其他重要性能因素。仿真结果表明,LHCP增益总是占总增益的主导地位。
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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