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Radar coverage predictions through time- and range-dependent refractive atmospheres with planetary boundary layer and electromagnetic parabolic equation models

机译:通过带行星边界层和电磁抛物线方程模型的时隙和范围依赖性屈光气氛的雷达覆盖预测

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The enhancement of the capability of electromagnetic parabolic equation (EMPE) and other propagation codes by using predictions from an atmospheric forecast model to provide refractivity data for range-dependent and time-varying situations is demonstrated. Starting from measured temperature and humidity data at one location and time, the JHU/APL planetary boundary layer model is used to obtained predictions for a 24-h forecast period. Predicted fields of temperature, humidity, and refractivity after 12 and 24 h are compared with measured data to verify the forecast, and vertical profiles of refractivity for each hour are provided, along with appropriate radar parameters, as input to EMPE. The EMPE calculations of expected radiation patterns as functions of height and range at selected times demonstrate the effects of hourly changes in the structure of the lower atmosphere on radar propagation. The radar propagation calculations have been repeated using the IREPS code to illustrate the similarities and differences between the two models when applied to this somewhat idealized, horizontally homogeneous situation.
机译:电磁抛物线方程(EMPE)和其他传播码的能力通过使用预测从大气预测模型以提供范围依赖性和时间变化的情况下,折射率数据增强是证明。在一个位置处和从时间测量的温度和湿度的数据开始,约翰霍普金斯大学/ APL行星边界层模型被用于为一个24小时的预测周期内获得的预测。 12个24小时后的温度,湿度,和折射率的预测字段与测量数据进行比较以验证预测,并且提供折射率为每个小时的垂直剖面,用适当的雷达参数一起,作为输入到EMPE。在选定的时间预期的辐射图案作为高度和范围的功能的EMPE计算表明的在低层大气中的雷达传播结构每小时变化的影响。使用IREPS代码时应用于此有些理想化,水平均匀的情况来说明两种模型之间的相似性和差异被重复使用雷达传播计算。

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