首页> 外文会议>Conference on microwave update >The Use of Sun, Quiet Sky and Earth Noise Measurements for Determining System Parameters, with Error Analysis
【24h】

The Use of Sun, Quiet Sky and Earth Noise Measurements for Determining System Parameters, with Error Analysis

机译:使用太阳,安静的天空和地球噪声测量来确定系统参数,具有错误分析

获取原文

摘要

The graphs of figures 4 and 5 apply the three-noise measurement scheme for determining system performance parameters, g/t, t and g. These are suitable for determining the performance, but perhaps a better method is the simple Basic program of Appendix I. The program quickly shows the specific answers for the measurements taken. The graphs are best for gaining insight about the method. One can see the way in which the performance parameters vary as the measurements vary. The program calculates the sensitivities for g/t, t_R (or t) and g to errors in the various input variables. A normalized sensitivity of 1 indicates that a small percentage error (or small dB error) in an input variable will resuk in the same percentage error (or dB error) in the performance parameter. Other values of the normalized sensitivity scale the parameters accordingly. After estimating the performance parameters, the sensitivities should be used to find the general order of magnitude of the errors. It is not generally necessary to make a statistical combination of the sensitivities. In order to compare system performance between different times, as well as to compare different systems, it is necessary to have obtained a value for the solar flux and the temperatures of the quiet sky and Earth. This requires a bit of extra effort, but allows a much more useful estimate than Sun-noise ratios. The step of computing g/t, t_R (or t) and g provides the most useful form of the answers. Finally, if the magnitude of the errors are estimated, it is possible to place statistical bounds on the performance parameters. Finally, here are some general rules for consideration: 1. Whenever taking Sun noise measurements, also take Earth noise measurements. 2. Obtain current solar flux numbers and interpolate for the frequency used. 3. Convert Sim noise into g/t values and use this as a primary measure of receiving performance. 4. Calculate the receiver and system noise temperatures. 5. Calculate the antenna gain, as it is the single parameter that relates to transmitter performance. 6. Try to estimate the errors in the measurements and parameters. 7. Keep the measurements in a notebook where they can be found when questions arise!
机译:图4和5的图形应用了三噪声测量方案,用于确定系统性能参数,G / T,T和G。这些都适用于确定性能,但也许更好的方法是附录I的简单基本程序。该程序快速显示了测量所采取的具体答案。图表最适合对该方法的洞察力。可以看到性能参数随测量变化而变化的方式。该程序计算各种输入变量中的G / T,T_R(或T)和G的敏感性。归一化的1表示输入变量中的小百分比误差(或小DB错误)将在性能参数中的相同百分比误差(或DB错误)中resuk。标准化灵敏度的其他值相应地缩放了参数。在估计性能参数后,应使用敏感度来查找错误的一般级。通常需要进行敏感性的统计组合。为了比较不同时间之间的系统性能,以及比较不同的系统,有必要获得太阳能通量的值和安静的天空和地球的温度。这需要一些额外的努力,但允许比太阳噪音比率更有用的估计。计算G / T,T_R(或T)和G的步骤提供了最有用的答案形式。最后,如果估计误差的幅度,则可以在性能参数上放置统计限制。最后,这里有一些一般规则供考虑:1。每当采取太阳噪声测量时,也会采取地球噪声测量。 2.获取当前的太阳能磁通号并插入用于使用的频率。 3.将SIM噪声转换为G / T值并使用此作为接收性能的主要测量。 4.计算接收器和系统噪声温度。 5.计算天线增益,因为它是与发射机性能相关的单个参数。 6.尝试估计测量和参数中的错误。 7.在问题出现问题时保持笔记本中的测量值。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号