Validation of Direction of Arrival with Orthogonal Tri-Dipole Antenna for SEAMS

H. A. Tanti, A. Datta
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引用次数: 1

Abstract

In this paper, validation of a fairly low computational complexity Direction of Arrival (DoA) estimation algorithm is done for a very low frequency antenna in context to an ongoing space mission Space Electric and Magnetic Sensor(SEAMS). The objective of this mission is to study low frequency emission from the Sun along with the Earth's magnetosphere & geo-tail, galactic & extra galactic spectra, 21 cm cosmology, and space plasma. To estimate the DoA a goniopolarimetric technique using 3 orthogonal dipole(tri-dipole) antennas are implemented. The tri-dipoles were simulated on CST simulation software with plane wave excitation for generating near realistic data for the DoA estimation. To estimate the frequency received at the tri-dipole antennas, the algorithm also utilizes Matrix pencil(MP) method and Least Square method(LSM).
正交三偶极子天线到达方向的验证
在本文中,验证了一个相当低的计算复杂度到达方向(DoA)估计算法在一个正在进行的空间任务空间电和磁传感器(seam)的背景下,对一个非常低频天线。该任务的目标是研究太阳的低频发射,以及地球的磁层和地尾,星系和星系外光谱,21厘米宇宙学和空间等离子体。为了估计DoA,实现了一种使用3个正交偶极子(三偶极子)天线的角极偏振测量技术。利用CST仿真软件对三偶极子进行了平面波激励模拟,得到了接近真实的DoA估计数据。为了估计三偶极子天线接收到的频率,该算法还采用了矩阵铅笔法和最小二乘法。
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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