Comparison of GPS TEC variations with IRI-2007 TEC prediction at equatorial latitudes during a low solar activity (2009-2011) phase over the Kenyan region

被引:42
|
作者
Olwendo, O. J. [1 ]
Baki, P. [2 ]
Cilliers, P. J. [3 ]
Mito, C. [4 ]
Doherty, P. [5 ]
机构
[1] Pwani Univ Coll, Sch Pure & Appl Sci, Dept Phys, Kilifi, Kenya
[2] Kenya Polytech Univ Coll, Sch Pure & Appl Sci, Dept Phys, Nairobi, Kenya
[3] Space Sci Directorate, South African Natl Space Agcy, Hermanus, South Africa
[4] Univ Nairobi, Dept Phys, Nairobi, Kenya
[5] Boston Coll, Inst Sci Res, Brighton, MA 02135 USA
关键词
GPS-TEC; IRI-2007; IRI-TEC; Equatorial anomaly; TOTAL ELECTRON-CONTENT; IONOSPHERIC VARIABILITY; SATELLITE; CREST;
D O I
10.1016/j.asr.2012.08.001
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
This work presents an analysis of the Total Electron Content (TEC) derived from the International GNSS Service (IGS) receivers at Malindi (ma12: 2.9 degrees S, 40.1 degrees E, dip -26.813 degrees), Kasarani (ram: 36.89 degrees E, 1.2 degrees S, dip -23.970 degrees), Eldoret (moiu: 35.3 degrees E, 0.3 degrees N, dip -21.037 degrees) and GPS-SCINDA (36.8 degrees E, 1.3 degrees S, dip -24.117 degrees) receiver located in Nairobi for the period 2009-2011. The diurnal, monthly and seasonal variations of the GPS derived TEC (GPS-TEC) and effects of space weather on TEC are compared with TEC from the 2007 International Reference Ionosphere model (IRI-TEC) using the NeQuick option for the topside electron density. The diurnal peaks in GPS-TEC is maximum during equinoctial months (March, April, October) and in December and minimum in June solstice months (May, June, July). The variability in GPS-TEC is minimal in all seasons between 0:00 and 04:00 UT and maximum near noon between 10:00 and 14:00 UT. Significant variability in TEC at post sunset hours after 16:00 UT (19:00 LT) has been noted in all the seasons except in June solstice. The TEC variability of the post sunset hours is associated with the occurrence of the ionization anomaly crest which enhances nighttime TEC over this region. A comparison between the GPS-TEC and IRI-TEC indicates that both the model and observation depicts a similar trend in the monthly and seasonal variations. However seasonal averages show that IRI-TEC values are higher than the GPS-TEC. The IRI-TEC also depicts a double peak in diurnal values unlike the GPS-TEC. This overestimation which is primarily during daytime hours could be due to the model overestimation of the equatorial anomaly effect on levels of ionospheric ionization over the low latitude regions. The IRI-TEC also does not show any response to geomagnetic activity, despite the STORM option being selected in the model; the IRI model generally remains smooth and underestimates TEC during a storm. The GPS-TEC variability indicated by standard deviation seasonal averages has been presented as a basis for extending the IRI-model to accommodate TEC-variability. (C) 2012 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1770 / 1779
页数:10
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