The first thermospheric neutral mass density model with robust and reliable uncertainty estimates is developed based on the SET HASDM density database. This database, created by Space Environment Technologies (SET), contains 20 years of outputs from the U.S. Space Force's High Accuracy Satellite Drag Model (HASDM), which represents the state-of-the-art for density and drag modeling. We utilize principal component analysis (PCA) for dimensionality reduction, creating the coefficients upon which nonlinear machine-learned (ML) regression models are trained. These models use three unique loss functions: mean square error (MSE), negative logarithm of predictive density (NLPD), and continuous ranked probability score (CRPS). Three input sets are also tested, showing improved performance when introducing time histories for geomagnetic indices. These models leverage Monte Carlo (MC) dropout to provide uncertainty estimates, and the use of the NLPD loss function results in well-calibrated uncertainty estimates without sacrificing model accuracy (<10% mean absolute error). By comparing the best HASDM-ML model to the HASDM database along satellite orbits, we found that the model provides robust and reliable uncertainties in the density space over all space weather conditions. A storm-time comparison shows that HASDM-ML also supplies meaningful uncertainty measurements during extreme events.
翻译:第一个大气中中性质量密度模型是建立在SETHASSDDM密度数据库基础上的,该数据库由空间环境技术(SET)创建,包含来自美国航天部队高精度卫星拖曳模型(HASDM)的20年产出,该模型代表了密度和拖动模型的先进性能。我们利用主要组成部分分析(PCA)来降低维度,创建用于培训非线性机器获取(ML)回归模型的参数。这些模型使用三种独特的损失函数:平均平方差(MSE)、预测密度负对数(NLPD)和连续排序概率分数(CRPS)。三个输入组也进行了测试,显示在引入地磁指数的时间历史时,业绩有所改善。这些模型利用蒙特卡洛(Monte Carlo)的辍学来提供不确定性估计,而使用NLPDD损失函数则导致在不牺牲模型准确性( < 10%表示绝对错误) 。通过将最佳的HADSDM-M模型与卫星轨道轨道上的最佳恒定度数据库进行比较,我们也在AMMDM事件期间提供了可靠的模型。