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Assessment of improvement of the IRI model over Ethiopia for the modeling of the variability of TEC during the period 2013-2016

机译:评估埃塞俄比亚IRI模型的改进以建模TEC在2013-2016年期间的变化

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This paper discusses the monthly and seasonal variation of the total electron content (TEC) and the improvement of performance of the IRI model in estimating TEC over Ethiopia during the solar maximum (2013-2016) phase employing as reference the GPS derived TEC data inferred from four GPS receivers installed in different regions of Ethiopia; Assosa (geog 10.05 degrees N, 34.55 degrees E, Geom. 7.01 degrees N), Ambo (8.97 degrees N, 37.86 degrees E, Geom. 5.42 degrees N), Nazret (8.57 degrees N, 39.29 degrees E, Geom. 4.81 degrees N) and Arba Minch (6.06 degrees N, 37.56 degrees E, Geom. 2.62 degrees N). The results reveal that, in the years 2013-2016, the highest peak GPS-derived diurnal VTEC is observed in the March equinox in 2015 over Arba Minch station. Moreover, both the arithmetic mean GPS-derived and modelled VTEC values, generally, show maximum and minimum values in the equinoctial and June solstice months, respectively in 2014-2015. However, in 2013, the minimum and maximum arithmetic mean GPS-derived values are observed in the March equinox and December solstice, respectively. The results also show that, even though overestimation of the modelled VTEC has been observed on most of the hours, all versions of the model are generally good to estimate both the monthly and seasonal diurnal hourly VTEC values, especially in the early morning hours (00:00-03:00 UT or 03:00-06:00 LT). However, it has also been shown that the IRI 2007 and IRI 2012 versions generally perform best in matching the diurnal GPS derived TEC values as compared to that of the IRI 2016 version. In addition, the IRI 2012 version with IRI2001 option for the topside electron density shows the highest overestimation of the VTEC as compared to the other options. None of the versions of the IRI model are proved to be able to capture the effects of geomagnetic storms. (C) 2018 COSPAR. Published by Elsevier Ltd. All rights reserved.
机译:本文讨论了总电子含量(TEC)的月度和季节变化以及IRI模型在太阳最大(2013-2016)阶段估算埃塞俄比亚TEC方面的性能改进,并参考了GPS推导的TEC数据在埃塞俄比亚不同地区安装了四个GPS接收器;阿萨萨(地理10.05度北,34.55度东,地理7.01度北),安博(8.97度,37.86度北,地理5.42度北),纳兹雷特(8.57度北,39.29度东,地理4.81度北) )和Arba Minch(北纬6.06度,东经37.56度,北纬2.62度)。结果表明,在2013-2016年期间,在2015年3月春分期间,在Arba Minch站观测到了GPS昼夜VTEC的最高峰值。此外,GPS的算术平均值和模型化的VTEC值通常分别在2014-2015年的等月和夏至月份显示最大值和最小值。然而,在2013年,分别在3月春分和12月冬至观测到GPS算术平均值的最小值和最大值。结果还表明,即使在大多数时间都观察到了模拟的VTEC的高估,该模型的所有版本通常都可以很好地估计每月和季节性的每日VTEC值,尤其是在清晨(00 :00-03:00 UT或03:00-06:00 LT)。但是,也已经显示,与IRI 2016版本相比,IRI 2007和IRI 2012版本通常在匹配昼夜GPS导出的TEC值方面表现最佳。此外,与其他选件相比,带有顶部电子密度的IRI2001选件的IRI 2012版本显示出对VTEC的最高估计。 IRI模型的任何版本都没有被证明能够捕获地磁风暴的影响。 (C)2018年COSPAR。由Elsevier Ltd.出版。保留所有权利。

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