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Prediction of Atmospheric Turbulence Refractive Index Structure Constant Based on Deep Learning

机译:基于深度学习的大气湍流折射率结构预测

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Aiming at the problem that atmospheric laser communication is easily affected by atmospheric turbulence, which will lead to the degradation of communication quality, RNN and LSTM were established based on deep learning to predict refractive index structure constant, one of the most important parameters of atmospheric turbulence. Based on it. reference for the selection of atmospheric laser communication channels can be provided to avoid waste of channel resources. Three statistical values average absolute error, root mean square error and correlation coefficient were used to analyze the prediction results. The results showed that both RNN and LSTM can predict very well under medium and strong turbulence. The correlation coefficient between the predicted data and the original data were 67.37% and 96.17%.
机译:针对大气激光通信容易受大气湍流影响的问题,这将导致通信质量的降低,RNN和LSTM基于深度学习来预测折射率结构恒定,是大气湍流最重要的参数之一。基于它。可以提供参考选择大气激光通信通道,以避免浪费信道资源。三个统计值平均绝对误差,均均方误差和相关系数用于分析预测结果。结果表明,RNN和LSTM都可以在中等和强大的湍流下预测得非常好。预测数据与原始数据之间的相关系数为67.37%和96.17%。

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