Characteristic Analysis of the Differences between TEC Values in GIM Grids

IF 1.7 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Qisheng Wang, Jiaru Zhu
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Abstract

Abstract. Using total electron content (TEC) from global ionosphere map (GIM) for ionospheric delay correction is a common method of eliminating ionospheric errors in satellite navigation and positioning. On this basis, the TEC of puncture point can be obtained by GIM grid TEC interpolation. However, in terms of grid, only few studies have analyzed the TEC value size characteristics of its four grid points, that is, the TEC difference characteristics among them. In view of this, by utilizing the GIM data from high solar activity years (2014) and low solar activity years (2021) provided by CODE, this paper proposes the grid TEC difference to analyze TEC variation characteristics within the grid, which is conducive to exploring and analyzing the variation characteristics of the ionosphere TEC in the single-station area. The results show that the TEC difference size within GIM grid is mainly related to the activity of ionosphere. The value is larger in high solar activity years and generally small in low solar activity years, and the value of high latitude area is always smaller than that of low latitude area. Specifically, in high solar activity years, most of the GIM grid TEC internal differences are within 4TECu in high and mid latitude regions, while only 78.17 % in low latitude regions; the grid TEC differences at 2-hour intervals are more scattered, and larger values occur in low latitude regions. In low solar activity years, the TEC difference values within GIM grid are mostly less than 2TECu, and most of them in the high and middle latitudes are within 1TECu. The GIM grid TEC difference values within 1-hour intervals are mostly less than 4TECu, and most of them in the high and middle latitudes are within 2TECu. The main finding of this analysis is that the grid TEC differences are small for most GIM grids, especially in the mid-high latitudes of low solar years. This means that relevant extraction methods and processes can be simplified when TEC within these GIM grids is needed.
GIM网格TEC值差异特征分析
摘要。利用全球电离层图(GIM)的总电子含量(TEC)进行电离层延迟校正是卫星导航定位中消除电离层误差的常用方法。在此基础上,通过GIM网格TEC插值得到穿刺点的TEC。然而,在网格方面,分析其四个网格点的TEC值大小特征,即它们之间的TEC差异特征的研究很少。鉴于此,本文利用CODE提供的太阳活动高年(2014年)和太阳活动低年(2021年)的GIM数据,提出栅格TEC差值分析栅格内TEC变化特征,有利于探索和分析单站区域电离层TEC的变化特征。结果表明,GIM网格内TEC差异大小主要与电离层活动有关。该值在太阳活动高年较大,在太阳活动低年一般较小,且高纬度地区的值始终小于低纬度地区。具体而言,在太阳活动高的年份,高纬度和中纬度地区GIM网格TEC内部差异大部分在4TECu以内,而低纬度地区只有78.17%;2 h栅格TEC差异较为分散,低纬度地区TEC差异较大。在太阳活动不活跃年,GIM网格内的TEC差值大多小于2TECu,高纬度和中纬度地区的TEC差值大多在1TECu以内。GIM格网1 h间隔内的TEC差值大多小于4TECu,高纬度和中纬度地区的TEC差值大多在2TECu以内。该分析的主要发现是栅格TEC差异在大多数GIM栅格中很小,特别是在低太阳年的中高纬度地区。这意味着当需要在这些GIM网格内进行TEC时,可以简化相关的提取方法和过程。
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来源期刊
Annales Geophysicae
Annales Geophysicae 地学-地球科学综合
CiteScore
4.30
自引率
0.00%
发文量
42
审稿时长
2 months
期刊介绍: Annales Geophysicae (ANGEO) is a not-for-profit international multi- and inter-disciplinary scientific open-access journal in the field of solar–terrestrial and planetary sciences. ANGEO publishes original articles and short communications (letters) on research of the Sun–Earth system, including the science of space weather, solar–terrestrial plasma physics, the Earth''s ionosphere and atmosphere, the magnetosphere, and the study of planets and planetary systems, the interaction between the different spheres of a planet, and the interaction across the planetary system. Topics range from space weathering, planetary magnetic field, and planetary interior and surface dynamics to the formation and evolution of planetary systems.
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