Temperature field reconstruction is essential for analyzing satellite heat reliability. As a representative machine learning model, the deep convolutional neural network (DCNN) is a powerful tool for reconstructing the satellite temperature field. However, DCNN needs a lot of labeled data to learn its parameters, which is contrary to the fact that actual satellite engineering can only acquire noisy unlabeled data. To solve the above problem, this paper proposes an unsupervised method, i.e., the physics-informed deep Monte Carlo quantile regression method, for reconstructing temperature field and quantifying the aleatoric uncertainty caused by data noise. For one thing, the proposed method combines a deep convolutional neural network with the known physics knowledge to reconstruct an accurate temperature field using only monitoring point temperatures. For another thing, the proposed method can quantify the aleatoric uncertainty by the Monte Carlo quantile regression. Based on the reconstructed temperature field and the quantified aleatoric uncertainty, this paper models an interval multilevel Bayesian Network to analyze satellite heat reliability. Two case studies are used to validate the proposed method.
翻译:温度场重建对于分析卫星热可靠性至关重要。 作为具有代表性的机器学习模型,深演神经网络(DCNNN)是重建卫星温度场的强大工具。 然而,DCNN需要大量标签数据来了解其参数,这与实际卫星工程只能获取噪音无标签数据的事实相反。为了解决上述问题,本文件提出一种不受监督的方法,即物理知情的深蒙特卡洛孔径回归法,用于重建温度场和量化由数据噪音造成的偏差不确定性。就一件事而言,拟议方法将深演神经网络与已知的物理知识结合起来,仅用监测点温度来重建准确的温度场。就另一件事,拟议方法可以量化蒙特卡洛孔蒂回归的偏差不确定性。根据重建后的温度场和量化的偏差不确定性,本文模型是一个用于分析卫星热可靠性的间隔多级贝伊斯网络。使用两个案例研究来验证拟议方法。