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不同强度磁暴期间热层大气密度响应特征分析

王昕 苗娟 刘四清 任廷领

王昕, 苗娟, 刘四清, 任廷领. 不同强度磁暴期间热层大气密度响应特征分析[J]. 空间科学学报, 2020, 40(1): 28-41. doi: 10.11728/cjss2020.01.028
引用本文: 王昕, 苗娟, 刘四清, 任廷领. 不同强度磁暴期间热层大气密度响应特征分析[J]. 空间科学学报, 2020, 40(1): 28-41. doi: 10.11728/cjss2020.01.028
WANG Xin, MIAO Juan, LIU Siqing, REN Tingling. Characteristics Analysis of Thermospheric Density Response during the Different Intensity of Geomagnetic Storms[J]. Chinese Journal of Space Science, 2020, 40(1): 28-41. doi: 10.11728/cjss2020.01.028
Citation: WANG Xin, MIAO Juan, LIU Siqing, REN Tingling. Characteristics Analysis of Thermospheric Density Response during the Different Intensity of Geomagnetic Storms[J]. Chinese Journal of Space Science, 2020, 40(1): 28-41. doi: 10.11728/cjss2020.01.028

不同强度磁暴期间热层大气密度响应特征分析

doi: 10.11728/cjss2020.01.028
基金项目: 

北京市科技重大专项资助(Z181100002918004)

详细信息
    作者简介:

    苗娟,E-mail:miaoj@nssc.ac.cn

  • 中图分类号: P352

Characteristics Analysis of Thermospheric Density Response during the Different Intensity of Geomagnetic Storms

  • 摘要: 利用CHAMP卫星数据,对2002-2008年12个不同强度磁暴事件期间的热层大气密度变化特征进行分析,并研究对应磁暴期间大气模式NRLMSISE-00分布特征.结果表明,大磁暴期间日侧大气密度峰值从高纬到低纬的时间延迟为2h,中小磁暴期间的延迟时间为3~4h;春秋季暴时大气密度分布基本呈南北对称分布,而夏冬季大气密度的分布是夏半球大于冬半球,春秋季暴时大气密度大于夏冬季;NRLMSISE-00大气模式得到的热层大气密度很好的体现了半球分布以及季节分布的特征,但模式模拟结果偏小;Dst指数峰值比ap指数峰值更能反应大气密度的变化情况.

     

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出版历程
  • 收稿日期:  2018-12-21
  • 修回日期:  2019-03-08
  • 刊出日期:  2020-01-15

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