利用COSMIC掩星数据监测电离层的异常变化

王虎; 刘志强; 白贵霞; 党亚民

doi:10.11728/cjss2014.01.046

利用COSMIC掩星数据监测电离层的异常变化

doi: 10.11728/cjss2014.01.046

王虎^1,3, ,,
刘志强^2,3,
白贵霞¹,
党亚民¹

1.
中国测绘科学研究院北京 100830
2.
河海大学地球科学与工程学院南京 210098
3.
同济大学测量与国土信息工程系上海 200092

基金项目: 国家自然科学基金项目（41374014，41174023）；北斗分析中心项目（GFZX0301040309）共同资助

详细信息

通讯作者:
王虎,E-mail:whxxf82@126.com

中图分类号: P352
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- 被引次数: 0
出版历程
- 收稿日期: 2012-12-24
- 修回日期: 2013-08-30
- 刊出日期: 2014-01-15

Monitoring of Ionospheric Anomaly Using COSMIC Occultation Measurementsormalsize

WANG Hu^{1,3
, ,},
LIU Zhiqiang^2,3,
BAI Guixia¹,
DANG Yamin¹

1.
Chinese Academy of Surveying and Mapping, Beijing 100830
2.
School of Earth Sciences and Engineering, Hohai University, Nanjing 210098
3.
Department of Surveying and Geo-informatics, Tongji University, Shanghai 200092

摘要

摘要: 分析了COSMIC掩星数据反演电子密度的方法，利用实例研究反演方法的特点，并采用ISR非相干散射雷达获取的电子密度数据进行验证，进而反演了长三角区域SHAO（IGS）站上空在日全食和太阳风暴期间的电子密度廓线图. 通过与平静日期间电离层电子密度进行比较，发现日全食及太阳风暴导致电离层发生的异常变化，从而提出COSMIC掩星数据反演电子密度在监测电离层变化时所具有的优势.
- COSMIC掩星 /
- 非相干散射雷达 /
- 电子密度
Abstract: The paper introduces the method of electron density inversion using COSMIC occultation data, and advantages of the inversion method are analyzed using practical calculation. Meanwhile, electron density profiles obtained from ISR (Incoherent Scattering Radar) are compared and analyzed with those from COSMIC occultation. Finally, electron density profiles over the SHAO (IGS station) which is located in Yangtze river region, are reversed using COSMIC occultation measurements during the total solar eclipse and the solar storm, and are compared with electron density profiles during the quite day. Ionospheric anomaly caused by the total solar eclipse and the solar storm are analyzed. The advantages of the inversion method from COSMIC occultation data have been found by using inversion method to monitor the ionosphere anomaly.
- COSMIC occultation /
- ISR (Incoherent Scattering Radar) /
- Electron density

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参考文献(8)

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