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GNSS derived TEC data ingestion into IRI 2012

机译:GNSS将TEC数据提取到IRI 2012中

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摘要

Experimental vertical total electron content (VTEC) data given by Global Ionospheric Maps (GIM) has been ingested into the IRI version 2012, aiming to obtain grids of effective input parameter values that allow to minimize the difference between the experimental and modeled vertical TEC. Making use of the experience gained with the technique of model adaptation applied to NeQuick (Nava et al., 2005), it has been found possible to compute IRI world grids of effective ionosphere index parameters (IG). The IG grids thus obtained can be interpolated in space and time to calculate with IRI the 3D electron density at any location and also the TEC along any ground-to-satellite ray-path for a given epoch. In this study, the ingestion technique is presented and a posteriori validation, along with an assessment of the capability of the 'ingested' IRI to reproduce the ionosphere day-to-day foF2 variability during disturbed and quiet periods. The foF2 values retrieved are compared with data from about 20 worldwide ionosondes for selected periods of high (year 2000) and moderate to low solar activity (year 2006). It was found that the use of the ingestion scheme enhances the performance of the model when compared with its standard use based on solar activity drivers (R12 and F10.7), especially for high solar activity. As an example, the mean and standard deviation of the differences between experimental and reconstructed F2-peak values for April of year 2000 is 0.09 and 1.28 MHz for ingested IRI, compared to -0.81 and 1.27 MHz (IRI with R12 input) and -0.02 and 1.46 MHz (IRI with F10.7 input).
机译:全球电离层地图(GIM)提供的实验性垂直总电子含量(VTEC)数据已被纳入IRI 2012版,旨在获得有效输入参数值的网格,从而最大程度地减少实验性和建模垂直TEC之间的差异。利用在NeQuick上应用模型自适应技术获得的经验(Nava等,2005),发现可以计算出有效电离层指数参数(IG)的IRI世界网格。可以在空间和时间上对由此获得的IG网格进行插值,以利用IRI计算给定历时在任何位置的3D电子密度,以及沿着任何地面到卫星射线路径的TEC。在这项研究中,提出了摄入技术并进行了后验验证,并评估了“被摄食的” IRI在扰动和安静时期重现电离层日常foF2变异性的能力。将取回的foF2值与选定的高强度(2000年)和中度至低太阳活动时间(2006年)的大约20个全球离子探空仪的数据进行比较。已经发现,与基于太阳活动驱动力(R12和F10.7)的标准使用相比,摄入方案的使用增强了模型的性能,尤其是对于高太阳活动。例如,对于摄入的IRI,2000年4月实验和重建F2峰值之间的差异的平均值和标准偏差为0.09和1.28 MHz,相比之下,-0.81和1.27 MHz(带R12输入的IRI)和-0.02和1.46 MHz(具有F10.7输入的IRI)。

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  • 来源
    《Advances in space research 》 |2015年第8期| 1994-2002| 共9页
  • 作者单位

    Telecommunications and ICT for Development Laboratory, Abdus Salam International Centre for Theoretical Physics (ICTP), Strada Costiera 11, 34151 Trieste (TS), Italy;

    Telecommunications and ICT for Development Laboratory, Abdus Salam International Centre for Theoretical Physics (ICTP), Strada Costiera 11, 34151 Trieste (TS), Italy;

    Telecommunications and ICT for Development Laboratory, Abdus Salam International Centre for Theoretical Physics (ICTP), Strada Costiera 11, 34151 Trieste (TS), Italy;

    Institute of Geophysics and Astronomy (IGA), La Habana, Cuba;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Ionospheric modeling; GNSS; TEC; Data ingestion; IRI;

    机译:电离层建模;GNSS;TEC;数据提取;IRI;

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