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The ionospheric polarisation of very low frequency radio waves.

机译:极低频无线电波的电离层极化。

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摘要

The lowest regions of the ionosphere are conveniently studied by means of reflection techniques using very low frequency radiowaves (10-30 kHz.).Most observations of this kind have measured only the cross polarised component of the reflected signal yielding the so-called conversion coefficient, R1. In this thesis an attempt is made to measure the in-plane signal, R, in addition to R1. From these two parameters the polarisation of the reflected waves may be determined. The results are interpreted in terms of the D-region electron density profiles by modelling techniques based on the full-wave analysis. Data collection for a period of one year are presented and discussed. A detailed account is given of the construction of equipment suitable for measurement of the normal polarised component of the ionospherically reflected radiowave, using the a modification of the 'loop and aerial' system. Due consideration is given to the experimental difficulties. It is established that the stability, both in phase and amplitude, is an extremely important factor in the success of the experiment. Methods are discussed of ensuring that no ground wave contamination exists, and details are given of a computer program to do this. A large section of the disertation is devoted to a detailed descrimption of the development of the data logging systems as these were responsible, to a large extent, for the success of the experimental programme. Of particular importance is the description of the on-line computing facility, using an advanced programmable calculator, with magnetic tape facility. The experimental data collected over one year is presented, and both seasonal and diurnal variations are presented. The related electron density profiles, derived by modelling the four measured paramenters, are discussed. Disturbed conditions have been considered for times of solar flare, stratospheric warmings and magnetic storm activity. Again modelling of profiles has been undertaken and a representative set is given. The necessity of measuring both, R and R1 for modelling work has been demonstrated and the errors likely to occur from using R1 alone have been fully discussed.
机译:电离层的最低区域可以通过使用非常低频率的无线电波(10-30 kHz)的反射技术方便地进行研究。大多数此类观测仅测量反射信号的交叉极化分量,从而产生所谓的转换系数。 ,R1。在本文中,除了R1之外,还尝试测量平面内信号R。根据这两个参数,可以确定反射波的偏振。通过基于全波分析的建模技术,可以根据D区电子密度分布来解释结果。介绍并讨论了为期一年的数据收集。使用“环路和天线”系统的改进形式,详细介绍了适用于测量电离层反射无线电波的正常极化分量的设备的结构。应适当考虑实验困难。已经确定,相位和幅度的稳定性是实验成功的极其重要的因素。讨论了确保不存在地波污染的方法,并详细说明了执行此操作的计算机程序。论文的大部分内容专门描述了数据记录系统的开发,因为这些在很大程度上对实验程序的成功负责。特别重要的是使用高级可编程计算器和磁带设备来描述在线计算设备。介绍了一年中收集的实验数据,并列出了季节和昼夜变化。讨论了通过对四个测量参数进行建模得出的相关电子密度分布。已经考虑到太阳耀斑,平流层变暖和磁暴活动时间受到干扰的条件。再次进行了轮廓建模,并给出了代表集。已经证明测量R和R1两者对于建模工作的必要性,并且已经充分讨论了仅使用R1可能发生的误差。

著录项

  • 作者

    Spracklen, Charles Timothy.;

  • 作者单位
  • 年度 1973
  • 总页数
  • 原文格式 PDF
  • 正文语种 {"code":"en","name":"English","id":9}
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