期刊文献+

风云四号A星和GOES-13相对论电子观测数据在轨交叉定标及数据融合研究 被引量:3

On-orbit cross-calibration and assimilation for relativistic electron observations from FengYun 4A and GOES-13
下载PDF
导出
摘要 地球磁层空间的相对论电子通过内部充放电效应,能够导致在轨航天器彻底失效.由于对这种空间粒子的特性和物理机制仍不清楚,磁层空间相对论电子一直是空间环境探测和空间科学研究的重要对象.开展相关磁层空间环境特性的研究和粒子辐射环境建模等,需要同时使用来自不同卫星、不同探测器的观测数据.消除不同探测器之间的系统偏差,实现不同来源数据的融合,是开展相关研究的必要前提.本文对我国最新的地球同步轨道卫星—风云四号A星(FY-4A)和同类轨道的美国GOES-13卫星相对论电子(>2 MeV)观测数据,开展在轨交叉定标及数据融合研究.本文严格筛选出地磁宁静期(Kp<2)的观测数据,以保证研究对象是被地磁场稳定捕获的辐射带粒子.根据辐射带粒子的物理特性,即3个绝热不变量的基础之上,以Liouville定理为依据,在漂移壳Lm坐标下比较两颗卫星观测到的电子通量,得到两颗卫星相对论电子观测之间的系统偏差.依据该结果,进行数据融合处理,结果表明系统偏差得以很好地消除.通过本项研究工作,得到了国际上重要的两个地球同步轨道相对论电子观测系统之间的偏差,并根据该研究成果,成功实现两个探测系统观测数据之间的融合,为后续的理论和应用研究工作打下了坚实的基础,也为地球同步轨道其他能道高能电子观测数据的在轨交叉定标和数据融合提供了参考方法. Magnetospheric relativistic electrons can destroy on-orbit spacecrafts completely by internal charging and discharging effects.As the characteristics and physical mechanism of this space particle are still unclear,magnetospheric relativistic electrons have always been an important object of space environment exploration and space science research.For studying the physical mechanisms and developing models relating to magnetospheric relativistic electrons,it is necessary to use the observations from different satellites and detectors at the same time.Eliminating the systematic deviation between different detection systems to assimilate the observations from different sources is essentially required by such researches.In this work,the onorbit cross-calibration and assimilation for relativistic electron(>2 MeV)observations from FengYun 4A and GOES-13 are performed.In this work,only the observations obtained under very quiet geomagnetic conditions(Kp<2)are adopted to ensure that the objects of study are the radiation belt particles,which are stably captured by the geomagnetic field.According to the physical characteristics of the radiation belt particles,that is,the three adiabatic invariants,and based on the Liouville theorem,the phase space density of the stably captured particles is unchanged.In this paper,the relativistic electron flux data of energy>2 MeV and instrument pitch angle are in the east and west direction respectively.If the particles’energy is the same,then their correspondingμvalues are the same,and their particles’directions are the same,then their corresponding J values are the same,and the Liouville theorem can be simplified as the drift shell Lm is the same,the fluxes are the same,and the electron fluxes observed by the two satellites are compared in the drift shell Lm coordinate.The systematic deviation between the two satellites’relativistic electronic observations can be obtained.According to this result,the data assimilation is carried out,and the results show that the system deviation can be removed well.By this research work,the systematic deviation between two important relativistic electron detection systems in geosynchronous orbit is obtained.Based on the obtained systematic deviations,the assimilations for observations from the two detection systems are achieved.This work lays a solid foundation for the follow-up theoretical and applied researches,and also provides the methods for on-orbit cross-calibration and observation assimilation which could be referred to when other electronic observations on geosynchronous orbit are dealt with.
作者 刘震 杨晓超 张效信 张珅毅 余庆龙 张鑫 薛炳森 郭建广 宗卫国 沈国红 白超平 周平 冀文涛 Liu Zhen;Yang Xiao-Chao;Zhang Xiao-Xin;Zhang Shen-Yi;Yu Qing-Long;Zhang Xin;Xue Bing-Sen;Guo Jian-Guang;Zong Wei-Guo;Shen Guo-Hong;Bai Chao-Ping;Zhou Ping;Ji Wen-Tao(National Space Science Center,Chinese Academy of Sciences,Beijing 100190,China;Beijing Key Laboratory of Space Environment Exploration,Beijing 100190,China;University of Chinese Academy of Sciences,Beijing 100190,China;Key Laboratory of Space Weather,National Center for Space Weather,Beijing 100081,China)
出处 《物理学报》 SCIE EI CAS CSCD 北大核心 2019年第15期350-356,共7页 Acta Physica Sinica
基金 国家自然科学基金(批准号:11603028)资助的课题~~
关键词 相对论电子 地球同步轨道 在轨交叉定标 数据融合 风云四号A星 relativistic electron geosynchronous orbit on-orbit cross-calibration data assimilation FengYun 4A
  • 相关文献

参考文献5

二级参考文献65

  • 1XIAO FuLiang1,2, CHEN LiangXu1, HE YiHua1 & YANG Chang1 1 School of Physics and Electronic Sciences, Changsha University of Science and Technology, Changsha 410004, China,2 State Key Laboratory of Space Weather, Chinese Academy of Sciences, Beijing 100190, China.Dynamic evolution of outer radiation belt electrons driven by superluminous R-X mode waves[J].Science China(Technological Sciences),2010,53(10):2734-2738. 被引量:7
  • 2邱科平,唐玉华,许敖敖.太阳软X射线观测进展[J].天文学进展,2004,22(3):227-234. 被引量:2
  • 3李秋莎,张柏荣.第22太阳周活动区M级以上X射线耀斑指数的统计[J].云南天文台台刊,1996(3):29-39. 被引量:5
  • 4孔令高,王世金,林华安,韦飞.FY-2C卫星太阳X射线探测器性能定标[J].空间科学学报,2006,26(5):370-376. 被引量:8
  • 5[1]Baker D N, Blake J B, Callis L B, et al. Relativistic electron acceleration and decay time scales in the inner and outer radiation belts: SAMPEX. Geophys Res Lett, 1994, 21: 409
  • 6[2]Li X, Baker D N, Temerin M D, et al. Are energetic electrons in the solar wind the source of the outer radiation belt? Geophys Res Lett, 1997, 24: 923
  • 7[3]Paulikas G A, Blake J B. Effects of the solar wind on magnetospheric dynamics: Energetic electrons at the synchronous orbit. In: Quantitative Model of Magnetospheric Processes, 21 Geophys Monograph Series, American Geophysical Union, Washington, DC, 1979
  • 8[4]Datlowe D. Relativistic electrons in solar particle events. Solar Phys, 1971, 17: 436
  • 9[5]Bothmer V, Posner A, Kunow H, et al. Solar energetic particle events and coronal mass ejections: New insights from SOHO. In: Wilson A, eds. Proceedings of the 31st ESLAB Symposium on Correlated Phenomena at the Sun. Noordwijk: ESA Publications Division, ESTEC, 1997. 207~216
  • 10[6]Gao Y F, Chi P J, Le G, et al. Sino-magnetic array at low latitudes (SMALL) including initial results from the sister sites in the United States. Adv Space Res, 1999, 25(7-7): 1343~1351

共引文献37

同被引文献21

引证文献3

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