利用土耳其全球导航卫星系统网络,基于经验正交函数建立电离层模型

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Kutubuddin Ansari , Janusz Walo , Selcuk Sagir , Kinga Wezka
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引用次数: 0

摘要

本研究调查了位于土耳其不同地区的五个选定全球导航卫星系统(GNSS)台站在土耳其上空的电离层总电子含量(TEC)变化情况。使用了地磁指数,并利用称为经验正交函数(EOF)的技术对观测到的 TEC 进行建模。值得注意的是,观测到的全球导航卫星系统 TEC 值与 EOF TEC 值之间的相关系数从 0.8020 到 0.9394 不等。观测到的 GNSS TEC 值与 EOF TEC 之间的均方根误差值介于 3.1665 TECU 与 4.4220 TECU 之间。这些结果表明,EOF 模型在土耳其地区的表现相当出色,能够完美地呈现模型的 TEC 变化。最后,对这些全球导航卫星系统观测值和 EOF 预测的 TEC 值以及地磁指数和对流层风速进行了研究。结果表明,观测到的和模型预测的 TEC 与对流层风速的相关性很低,没有提供任何显著值。因此,我们得出结论,电离层区域不受对流层风速的影响。这是因为对流层风速与对流层下部及其大气压力有关,而电离层远离地球,取决于自由电子的数量。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Empirical orthogonal function based modelling of ionosphere using Turkish GNSS network

The study investigates ionospheric total electron content (TEC) variation over Turkey from the five selected global navigation satellite system (GNSS) stations situated in diverse parts of Turkey. The geomagnetic indices are used and observed TEC are modeled with the technique known as Empirical orthogonal function (EOF). It is valuable to note that the correlation coefficient between observed GNSS TEC values and EOF TEC values varies from 0.8020 to 0.9394. The root means square error (RMSE) values between observed GNSS TEC values and EOF TEC lie between 3.1665 TECU to 4.4220 TECU. These results show that the EOF model performs quite well in the Turkish region and can present the model TEC variations perfectly. Finally, these GNSS observed and EOF-predicted TEC values along with geomagnetic indices are studied with the tropospheric wind speed. The results showed that both observed and modeled TEC have very low correlations with tropospheric wind speed and do not provide any significant value. Hence, we concluded that the ionospheric region is not affected by tropospheric wind speed. It happens because the tropospheric wind speed is a matter of the lower troposphere and its atmospheric pressure while the ionosphere is far from the earth and depends upon the number of free electrons.

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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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