首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Modeling of Topside Ionospheric Vertical Scale Height Based on Ionospheric Radio Occultation Measurements
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Modeling of Topside Ionospheric Vertical Scale Height Based on Ionospheric Radio Occultation Measurements

机译:基于电离层无线电掩星测量的顶侧电离层垂直尺度高度建模

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摘要

An artificial neural network (ANN) method for the modeling of global topside ionospheric vertical scale height (VSH) using electron density profiles retrieved from Global Navigation Satellite Systems radio occultation (RO) data is proposed in this study. The data for this study are 80,124 VSHs derived from the events randomly selected from 9 years of Constellation Observing System for Meteorology, Ionosphere, and Climate RO measurements and 144,530 VSHs derived from the events randomly selected from 16 years of topside sounder measurements of both Aluoette-1/2 and ISIS-1/2 satellites during 1962-1978 are used for comparison. VSHs from the International Reference Ionosphere are also used for the comparison. Results showed that: (1) the median of the relative residuals of the new ANN regression approach/model (which was based on RO measurements) was 8.5% less than that of the traditional approach/model (which was based on the topside sounder data);(2) the median of the relative residuals of the ANN model when longitude was used as a variable was 1.1% less than the one without longitude;and substantial error in the polar region was shown to be mitigated by taking the variable longitude into consideration;(3) compared to International Reference Ionosphere, the accuracy of the new ANN model was improved by around 14%;(4) the new ANN model outperforms the traditional base vector-based least squares model by around 10% when incoherent scatter radar measurements are used as a reference;and (5) the characteristics of global VSHs generated from the new model during geomagnetic storms better agree with measurements than that of the base vector-based least squares.
机译:在本研究中提出了使用从全球导航卫星系统无线电掩星(RO)数据检索的电子密度分布的全局顶侧电离层垂直尺度高度(VSH)的人工神经网络(VSH)。本研究的数据是80,124 VSHS来自于从9年的星座观察系统中源于气象,电离层和气候RO测量的事件,144,530 vshs从aluoette的16年中随机选择的事件中衍生出来的事件 - 1962-1978期间的1/2和Isis-1/2卫星用于比较。来自国际参考电离层的VSH也用于比较。结果表明:(1)新的ANN回归方法/型号(基于RO测量)的相对残留的中位数为8.5%,比传统方法/型号(这是基于顶部发声器数据) );(2)ANN模型的相对残差的中值作为变量的时间为1.1%,比没有经度的1%小;通过将可变经度进行可变经度来减轻极性区域的大量误差考虑;(3)与国际参考电离层相比,新的ANN模型的准确性提高了约14%;(4)新的ANN模型在不连贯的散射雷达时达到了大约10%的传统基础向量的最小二乘型号。测量用作参考;(5)从地磁风暴期间从新模型生成的全局VSH的特征更好地同意比基于基于载体的最小二乘法的测量值。

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  • 作者单位

    SPACE Research Centre School of Science RMIT University Melbourne Australia;

    SPACE Research Centre School of Science RMIT University Melbourne Australia;

    SPACE Research Centre School of Science RMIT University Melbourne Australia;

    SPACE Research Centre School of Science RMIT University Melbourne Australia;

    SPACE Research Centre School of Science RMIT University Melbourne Australia;

    Academy of Opto-Electronics Chinese Academy of Sciences Beijing China;

    School of Environmental Science and Spatial Informatics China University of Mining and Technology Xuzhou China;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 空间物理;
  • 关键词

    modeling; randomly; events;

    机译:建模;随机;事件;

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