Ionospheric temporal variations over the region of Turkey: a study based on long-time TEC observations

被引:0
作者
Erman Şentürk
Murat Selim Çepni
机构
[1] Kocaeli University,Department of Surveying Engineering
来源
Acta Geodaetica et Geophysica | 2018年 / 53卷
关键词
CODE–GIM; Mid-latitude; Ionosphere; Space-weather; Temporal variation;
D O I
暂无
中图分类号
学科分类号
摘要
In this study, daily mean vertical total electron content (VTEC) and daily mean 2-h VTEC values were obtained from Center for Orbit Determination in Europe–Global Ionosphere Maps (CODE–GIM) data over the region of Turkey between January 1, 2003, and December 31, 2016. The time interval is sufficient to reflect temporal changes of the ionosphere. The daily mean VTEC data was used to analyze the space weather effects on the VTEC variability and daily mean 2-h VTEC data was utilized to see the pattern of the diurnal, monthly, seasonal and yearly variation of VTEC values. The highest correlation was found between VTEC and F10.7 (r = 0.83). Totally, 40 major geomagnetic storms were identified that 45% of the storms are caused a decrease and 55% of the storms are caused an increase in VTEC variation. The maximum VTEC is shown at 13:00 LT and the minimum VTEC is shown at 03:00 LT according to diurnal variation of the 14-year mean 2-h VTEC. The maximum VTEC is shown on April and the minimum VTEC is shown on July according to diurnal variation of monthly mean VTEC. Diurnal variation of seasonal mean VTEC and its standard deviations are higher in equinox than solstices. Diurnal variation of yearly mean VTEC has a significant change from low to high solar activity periods.
引用
收藏
页码:623 / 637
页数:14
相关论文
共 110 条
[1]  
Adeniyi JO(2013)Determination of the threshold value of F10.7 in the dependence of foF2 on solar activity Adv Space Res 51 1709-1714
[2]  
Ikubanni SO(2017)Analysis of ionospheric TEC from GNSS observables over the Turkish region and predictability of IRI and SPIM models Astrophys Space Sci 362 65-1057
[3]  
Ansari K(2009)TEC variations during low solar activity period (2005–2007) near the equatorial ionospheric anomaly crest region in India Ann Geophys 27 1047-120
[4]  
Corumluoglu O(2012)Solar EUV flux (0.1–50 nm), F10.7 cm flux, sunspot number and the total electron content in the crest region of equatorial ionization anomaly during the deep minimum between solar cycle 23 and 24 Indian J Radio Space Phys 41 110-14
[5]  
Panda SK(2017)Ionospheric F-region observations over American sector during an intense space weather event using multi-instruments J Atmos Solar Terr Phys 156 1-70
[6]  
Bagiya MS(1969)F-region seasonal and magnetic storm behaviour J Atmos Terr Phys 31 59-1125
[7]  
Joshi HP(1969)The hysteresis variation in F2-layer parameters J Atmos Terr Phys 31 1119-342
[8]  
Iyer KN(2015)Temporal–spatial variation of global GPS-derived total electron content, 1999–2013 PLoS ONE 10 e0133378-1084
[9]  
Aggarwal M(2015)Monitoring ionospheric variation for a definite period time in Turkey Int Arch Photogramm Remote Sens Spat Inf Sci 40 339-1324
[10]  
Ravindran S(2005)Ionospheric space weather effects monitored by simultaneous ground and space based GNSS signals J Atmos Sol Terr Phys 67 1074-178