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大气密度模型球谐修正研究

任廷领 苗娟 刘四清 王宏 曹勇

任廷领, 苗娟, 刘四清, 王宏, 曹勇. 大气密度模型球谐修正研究[J]. 空间科学学报, 2019, 39(4): 442-448. doi: 10.11728/cjss2019.04.442
引用本文: 任廷领, 苗娟, 刘四清, 王宏, 曹勇. 大气密度模型球谐修正研究[J]. 空间科学学报, 2019, 39(4): 442-448. doi: 10.11728/cjss2019.04.442
REN Tingling, MIAO Juan, LIU Siqing, WANG Hong, CAO Yong. Spherical Calibration Method on Atmospheric Density Model[J]. Chinese Journal of Space Science, 2019, 39(4): 442-448. doi: 10.11728/cjss2019.04.442
Citation: REN Tingling, MIAO Juan, LIU Siqing, WANG Hong, CAO Yong. Spherical Calibration Method on Atmospheric Density Model[J]. Chinese Journal of Space Science, 2019, 39(4): 442-448. doi: 10.11728/cjss2019.04.442

大气密度模型球谐修正研究

doi: 10.11728/cjss2019.04.442 cstr: 32142.14.cjss2019.04.442
基金项目: 

深圳科技计划项目资助(JCYJ20160817172025986)

详细信息
    作者简介:
    • 任廷领,rentl@nssc.ac.cn
  • 中图分类号: P354

Spherical Calibration Method on Atmospheric Density Model

  • 摘要: 大气模型修正是提高模型精度的一种重要方法.利用CHAMP卫星高精度加速仪反演的密度数据,采用球谐函数的形式对NRLMSISE-00模型进行修正.为了消除轨道高度变化对密度修正结果的影响,将密度数据同化到同一高度处,计算修正之后的密度误差,进而对未来三天的密度进行预报.结果表明,经球谐修正后,修正误差和预报误差均有显著降低.在太阳活动高年,修正误差可降至10%左右,提前1~3天预报精度分别提高31.34%,21.39%和13.75%;太阳低年时修正误差可降至14%左右,提前1~3天预报精度分别提高55.03%,47.79%和43.60%.

     

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出版历程
  • 收稿日期:  2018-06-05
  • 修回日期:  2019-05-22
  • 刊出日期:  2019-07-15

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