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Temporal-frequency spectra for plane and spherical waves in a millimetric wave absorption band

机译:毫米波吸收带中的平面波和球面波的时频谱

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摘要

Complete analytical expressions for the temporal power spectral density functions in a millimetric wave absorption region for plane and spherical waves have been developed for both amplitude and phase fluctuations due to atmospheric turbulence. Asymptotic expressions for both high and low scintillation frequencies are derived. Theoretical expressions for the differential phase power spectrum (i.e. the phase difference between two frequencies) are also presented. Experimental results of amplitude and differential phase scintillations measured on a 4.1-km link across central London, are presented. Results show that the plane wave case gives the best agreement with theory for this particular link. It is also shown that neglecting the cross-spectral density term at the higher scintillation frequencies for the differential phase spectrum can lead to a large difference between the theoretical and experimental power spectra. In particular, for a small frequency separation and a large value of the outer scale of turbulence, the highest scintillation frequencies are too low to neglect the cross term.
机译:对于大气湍流引起的振幅和相位波动,已经针对平面波和球面波的毫米波吸收区域中的时间功率谱密度函数开发了完整的解析表达式。导出了高和低闪烁频率的渐近表达式。还给出了差分相位功率谱(即两个频率之间的相位差)的理论表达式。呈现了在整个伦敦市中心4.1公里的链路上测得的幅度和相位微闪烁的实验结果。结果表明,对于这种特定的联系,平面波情况与理论具有最佳的一致性。还显示出,对于较高的闪烁频率,对于差分相位谱,忽略互谱密度项会导致理论功率谱和实验功率谱之间的较大差异。特别是对于较小的频率间隔和较大的外部湍流尺度,最高的闪烁频率太低而无法忽略交叉项。

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