Maximum Usable Frequencies for Radio Sky-Wave Transmission, 1933 to 1937

T. R. Gilliland, S. S. Kirby, N. Smith, S. E. Reymer
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引用次数: 5

Abstract

Graphs are presented to indicate the maximum usable frequencies for sky-wave transmission from June, 1933, to December, 1937. The graphs are given for March, June, and December to show equinoctial, summer, and winter conditions for each year. The factors which must be considered in deriving these graphs from vertical-incidence ionosphere measurements are outlined briefly. The principal factors are Snell's law, variation of virtual height of the ionosphere with frequency, the curvature of the ionosphere, and the effect of the earth's magnetic field. The method of applying these graphs to simple and complex transmission paths is indicated. The effect of sporadic E reflections, absorption, and scattered reflections are discussed briefly. In conclusion it is pointed out that the graphs and the ionosphere data, from which they were derived, may be used to estimate future diurnal, seasonal, and longtime variations of maximum usable frequencies.
无线电天波传输的最大可用频率,1933至1937年
图表显示了1933年6月至1937年12月天波传输的最大可用频率。图表给出了3月、6月和12月的情况,以显示每年的分点、夏天和冬天的情况。在从垂直入射电离层测量得到这些图时必须考虑的因素作了简要概述。其主要影响因素有斯涅尔定律、电离层虚高随频率的变化、电离层曲率和地磁场的影响。给出了将这些图应用于简单和复杂传输路径的方法。简要讨论了散射反射、吸收和散射反射的影响。最后指出,图表和电离层资料可用于估计未来最大可用频率的日变化、季节变化和长期变化。
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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