Volume 46 Issue 2
Jan.  2021
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FENG Jiandi, ZHAO Zhenzhen, HAN Baomin, ZHONG Huixin, ZHU Yuncong. A Single-Station Empirical TEC Model Suitable for MSNA Area: Taking ohi3 Station as an Example[J]. Geomatics and Information Science of Wuhan University, 2021, 46(2): 270-279,288. DOI: 10.13203/j.whugis20190211
Citation: FENG Jiandi, ZHAO Zhenzhen, HAN Baomin, ZHONG Huixin, ZHU Yuncong. A Single-Station Empirical TEC Model Suitable for MSNA Area: Taking ohi3 Station as an Example[J]. Geomatics and Information Science of Wuhan University, 2021, 46(2): 270-279,288. DOI: 10.13203/j.whugis20190211
shu

A Single-Station Empirical TEC Model Suitable for MSNA Area: Taking ohi3 Station as an Example

  • 1.

    School of Civil and Architectural Engineering, Shandong University of Technology, Zibo 255000, China

  • 2.

    Shanghai Key Laboratory of Space Navigation and Positioning Techniques, Shanghai 200030, China

  • 3.

    School of Geodesy and Geomatics, Wuhan University, Wuhan 430079, China

Funds: 

The National Natural Science Foundation of China 41804032

the Open Fund of State Key Laboratory of Geodesy and Earth's Dynamics SKLGED2019-3-4-E

the Open Fund of Shanghai Key Laboratory of Space Navigation and Positioning Techniques 201920

More Information
  • Author Bio:

    FENG Jiandi, PhD, lecturer, specializes in GNSS data processing and ionospheric model. E-mail: jdfeng@whu.edu.cn

  • Corresponding author:

    HAN Baomin, PhD, professor. E-mail: hanbm@sdut.edu.cn

  • Received Date: September 29, 2019
  • Published Date: February 04, 2021
    Graphical Abstract
    • Abstract
  • The diurnal variability of total electron content (TEC) in midlatitude summer nighttime anomaly (MSNA) region varies seasonally. Whether the characteristics of MSNA can be effectively described is one of the key indicators to test the accuracy of ionospheric empirical TEC model. A new ionospheric empirical TEC model named SSM-T2 (single station model type2) is proposed for MSNA anomalies. The effectiveness of the model is verified by an example of ohi3 located in the Antarctic Peninsula in the MSNA region. The SSM-T2 model consists of three parts: The diurnal variation component of TEC, the seasonal variation component and the solar activity component. The coefficients in the model are obtained by least square fitting. At the ohi3 station in the Antarctic Peninsula, test results of the model fitting show that the SSM-T2-ohi3 model fits well with the modeling data GPS-TEC, and describes the MSNA phenomenon well. By comparing and analyzing the models, it is found that SSM-T2-ohi3 is in good agreement with CODE GIMs (Center for Orbit Determination in Europe, Global Ionosphere Maps) and SSM-month models at extrapolated time points. It can effectively describe the characteristics of MSNA and has better prediction ability than IRI2016 model.
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    • References (45)
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