临近空间大气密度时空扰动规律及建模研究  

STUDY OF THE TEMPORAL-SPATIAL FLUCTUATIONS AND EMPIRICAL MODEL OF NEAR SPACE ATMOSPHERIC DENSITY

作　　者：曾丹丹 万田[1,2] 李帅辉 Zeng Dandan;Wan Tian;Li Shuaihui(State Key Laboratory of High Temperature Gas Dynamics,Institute of Mechanics,Chinese Academy of Sciences,Beijing 100190,China;School of Engineering Science,University of Chinese Academy Sciences,Beijing 100049,China)

机构地区：[1]中国科学院力学研究所高温气体动力学国家重点实验室,北京100190 [2]中国科学院大学工程科学学院,北京100049

出　　处：《力学学报》2022年第11期2984-2993,共10页Chinese Journal of Theoretical and Applied Mechanics

摘　　要：大气密度是飞行器能源动力设计、飞行控制中的重要输入参数.近年来,多项研究发现,对于临近空间高层大气,常用经验模型如USSA-76, NRLMSISE-00的密度预示值偏大.另外,随着飞行器精细化设计趋势,要求经验模型可预示不同纬度、昼夜和季节条件下的密度特性.基于此,本文利用卫星观测数据全面分析了临近空间大气密度随纬度、地方时、日期的变化规律,包括变化模式和变化幅度.纬度、日期引起的变化幅度大于地方时引起的变化幅度.纬度、日期引起的密度变化在不同高度范围表现出不同模式;变化幅度在78 km附近达最大值,在22 km和92 km附近达局部极小值.地方时引起的密度变化随高度递增.根据大气密度的时空变化特性,本文提出了临近空间大气密度的时空扰动模型,该模型能描述临近空间大气密度及其随纬度、地方时、日期的变化规律.与以往经验模型相比,时空扰动模型可更好地描述不同高度下密度的时空变化规律.在相同误差带条件下,本文模型的置信度明显优于NRLMSISE-00.本文建模方法合理,模型结果对临近空间飞行器设计有应用价值.Atmospheric density is a fundamental parameter for vehicle designing and flight controlling. In recent years,many researchers have discovered that atmospheric densities in the upper mesosphere and lower thermosphere predicted by the empirical model, such as USSA-76 and NRLMSISE-00, are larger than the measured values. On the other hand,vehicle designing is tending to be more detailed, and engineers hope that the empirical models provide densities under variable latitudes, day-night times and seasons. Based on that, the present work analyzesdependences of near-space atmospheric density on latitude, solar local time and date, by using satellite observed data. Emphasizes are put on density fluctuation patterns and amplitudes. The fluctuation patterns caused by latitude and date vary with altitude, and the amplitudes are largest at 78 km and locally smallest at about 22 km and 92 km. The fluctuation amplitude caused by the solar local time increases monotonically with altitude. Based on the temporal-spatialfluctuationlaw, we proposed the temporal-spatial fluctuation modelfor the near-space atmospheric density, which describes the density fluctuations with latitude, local time and date. The present model describes the temporal-spatial fluctuations better than the existed empirical models at variable altitudes. The confidence coefficient of the present model is much better than NRLMSISE-00under the same error band. The modeling method in this work is reasonable, and the obtained model could be used in near-space vehicle designing.

关 键 词：临近空间大气密度 时空扰动规律 卫星观测数据 经验模型 

分 类 号：P432.2[天文地球—大气科学及气象学]