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Novel Compact Model for the Radiation Pattern of UWB Antennas Using Vector Spherical and Slepian Decomposition

机译:基于矢量球面和Slepian分解的UWB天线辐射方向图的紧凑模型

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A new compact model is described for the 3D radiation pattern of an ultrawideband antenna, using a vector spherical and Slepian decomposition. Vector spherical modes are known to provide a good basis for the angular dependency of the radiation pattern. This paper is the first to extend such a model to also incorporate the frequency dependency of a radiation pattern. This is achieved by using a Slepian mode expansion. It is shown that this model requires considerably less coefficients than traditional sampling to accurately describe a frequency-dependent 3D radiation pattern. Also, generating the Slepian modes is computationally more efficient than comparable techniques, such as the singularity expansion method (SEM). The coefficients can then directly be used to efficiently calculate performance measures such as the antenna Fidelity Factor for all angles $(phi,theta )$ without reconstructing the radiation pattern, or to reduce the noise contribution.
机译:描述了一种新的紧凑模型,该模型使用矢量球面和斯利普式分解,用于超宽带天线的3D辐射方向图。已知矢量球形模式为辐射方向图的角度依赖性提供了良好的基础。本文是第一个扩展这种模型以包含辐射方向图的频率依赖性的论文。这可以通过使用Slepian模式扩展来实现。结果表明,与传统采样相比,该模型所需的系数要少得多,以准确描述频率相关的3D辐射方向图。同样,生成Slepian模式比类似技术(例如奇异扩展方法(SEM))在计算上更高效。然后,可以将该系数直接用于有效地计算性能度量,例如针对所有角度$(phi,θ)$的天线保真度因子,而无需重构辐射图,或减少噪声贡献。

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