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Modeling the Spatio-Temporal Variability of the Atmospheric Refractive Index in Optical Measurements

机译:在光学测量中模拟大气折射率的时空变化

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The paper proposes approaches and mathematical models for assessing the spatio-temporal variability of the refractive index of the atmosphere during optical measurements. In the calculations, such characteristics of temperature-wind sounding of the atmosphere as temperature and humidity, atmospheric pressure, etc. are used. The obtained mathematical models allow restoring the field of the atmospheric refractive index, which is subject to strong changes in the surface layer. Accordingly, taking into account the obtained data leads to a decrease in the error of optical measurements, which reaches a maximum on inclined paths, where the path of observation of objects differs from a straight line. The initial information for the calculations are: the values and magnitudes of the gradient of the refractive index, as well as the viewing angles of the object relative to the normal. Using mathematical models, the numerical values of possible errors are calculated, which is necessary to adjust the results of optical measurements.
机译:本文提出了评估光学测量过程中大气折射率的时空变化的方法和数学模型。在计算中,使用诸如温度和湿度,大气压等的大气的温度-风探测特性。所获得的数学模型允许恢复大气折射率的场,该大气场在表层中发生强烈变化。因此,考虑所获得的数据导致光学测量误差的减小,该误差在倾斜的路径上达到最大值,在该倾斜的路径上,物体的观察路径不同于直线。用于计算的初始信息是:折射率梯度的值和大小,以及物体相对于法线的视角。使用数学模型,计算可能的误差的数值,这是调整光学测量结果所必需的。

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