期刊文献+

碰撞风险评估中的空间环境激励图方法

Space environmental excitation graph method for collision risk assessment
下载PDF
导出
摘要 因航天器物理特征、空间环境扰动变化、预报技术和大气模型性能等既有不确定因素的存在,空间目标碰撞概率等与轨道预报相关的评估工作存在模糊度问题,无法准确描述碰撞风险水平。文章基于碰撞概率极值,简化气动力误差模型,量化计算轨道预报相关事务的边界;提出空间环境激励图和3σ区的概念,并给出具体实施方法以及空间碎片碰撞预警、空间物体陨落预报的计算示例。计算结果表明,该方法能较好应对轨道预报相关事务中的模糊度问题,可为相关航天工程实践和决策提供参考。 Due to the factors of uncertainty,such as those in the spacecraft physical characteristics,the disturbance of the space environment,the space environment prediction technique,and the performance of the atmospheric model,the assessments for the space target collision probability related to the orbit prediction may not be clear enough to accurately describe the collision rate levels.In this paper,based on the extreme value of the collision probability,the aerodynamic force error model is simplified and the boundary of the orbit prediction related issues is calculated quantitatively.The concepts of the spatial environment excitation graph and the 3σdomain are proposed,and the corresponsive method is implemented with calculation example of the space debris collision warning and the forecast of the fall-to-Earth of space objects.It is shown that the method can be used to evaluate and deal with the ambiguity problems in the orbit prediction related work,to provide some guidance for the relevant decision-making in the aerospace engineering practice.
作者 刘卫 石晟玮 罗冰显 刘舒莳 刘四清 龚建村 钟秋珍 LIU Wei;SHI Shengwei;LUO Bingxian;LIU Shushi;LIU Siqing;GONG Jiancun;ZHONG Qiuzhen(National Space Science Center,Chinese Academy of Sciences,Beijing 100190,China;Beijing Institute of Tracking and Telecommunications Technology;Beijing Aerospace Control Center,Beijing 100094,China;Innovation Academy for Microsatellites,Chinese Academy of Sciences,Shanghai 201210,China;University of Chinese Academy of Sciences,Beijing 100049,China)
出处 《航天器环境工程》 北大核心 2022年第5期482-488,共7页 Spacecraft Environment Engineering
基金 中国科学院重点部署项目(编号:ZDRE-KT-2021-3)。
关键词 空间环境 激励图 碰撞预警 碰撞概率 模糊度 space environment excitation method collision warning collision probability ambiguity
  • 相关文献

参考文献2

二级参考文献18

  • 1徐天河,杨元喜.利用现有重力场模型求定CHAMP卫星加速度计修正参数[J].测绘学报,2004,33(3):200-204. 被引量:10
  • 2钟秋珍,刘四清,何卷雄,龚建村.奇异谱分析在太阳10.7cm射电流量中期预测中的应用[J].空间科学学报,2005,25(3):199-203. 被引量:7
  • 3马瑞平,纪巧,徐寄遥.太阳F_(10.7)指数准27天振荡的小波分析[J].空间科学学报,2007,27(2):89-95. 被引量:9
  • 4Christiansen W N, Yabsley D E, Mills B Y. Measurements of Solar Radiation at a Wavelength Of 50 Centimetres During the Eclipse of November 1, 1948. Aust. J. Sci. Res., 1949. A2:506.
  • 5Jeongwoo L. Radio emissions from solar active regions [J]. Space Sci. Rev., 2007, 133:73-102.
  • 6Alissandrakis C E. A model for sunspot associated emission at 6cm wavelength [J]. Astron. Astrophys., 1980, 82:30-40.
  • 7Jacchia L G. New static models of the thermosphere and exosphere with empirical temperature profiles [R]. Smith-sonian Astrophysics Special Report 313, 1970.
  • 8Jacchia L G. Revised static model of the thermosphere and exosphere with empirical temperature profiles [R]. Smith: sonian Astrophysics Special Report 332, 1971.
  • 9Jacchia L G. Thermospheric temperature, density, and composition: new models [R]. Smithsonian Astrophysics Special Report 375, 1977.
  • 10Hedin A E. Extension of the MSIS thermosphere model into the middle and lower atmosphere [J]. J. Geophys. Res., 1992, 96:1159-1172.

共引文献11

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部