Variability of Equatorial Electrojet (EEJ) at EIA regions

L. Olatunbosun, A. Olabode, E. Ariyibi
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Abstract

The EEJ is a worldwide solar-driven wind that results in the solar quiet (Sq) current system in the E region of the earth’s ionosphere. The variability of some features such as EEJ, are very important in understanding the complex nature of the ionosphere, especially the low-latitude ionosphere. The magnetometer data from stations located near the equator and outside the edge of the electrojet strip for Africa and India stations were used to estimate and investigate the variability of EEJ in African and Indian Low-Latitudes. The stations are Addis Ababa, Ethiopia (geographic lat/long: 9.03oN/38.76oE) and at Mbour, Senegal for African region (geographic lat/long 14.392oN/343.042oE) and Hyderabad, India (geographic lat/long: 17.413oN/78.555oE) and Beijing Ming Tombs, China for Indian region (geographic lat/long: 40.3oN/116.2oE). The data in XYZ orientation was used to estimate the EEJ strength. The result shows that EEJ exhibits diurnal and seasonal variations and that its variability is stronger in African station than in Indian station, so also is the occurrence of counter electrojet (CEJ).
赤道电喷流(EEJ)在EIA区域的变率
EEJ是一种全球性的太阳能驱动风,它在地球电离层的E区产生太阳静(Sq)电流系统。一些特征的变率,如EEJ,对于理解电离层,特别是低纬度电离层的复杂性质非常重要。利用非洲和印度站赤道附近和电喷带边缘外的磁力计资料,估计和研究了非洲和印度低纬度地区EEJ的变率。分别位于埃塞俄比亚亚的斯亚贝巴(地理纬度:9.03oN/38.76东经)、塞内加尔Mbour(地理纬度:14.392oN/343.042东经)、印度海得拉巴(地理纬度:17.413oN/78.555东经)和中国北京十三陵(地理纬度:40.3oN/116.2东经)。XYZ方向的数据用于估计EEJ强度。结果表明,EEJ具有明显的日变化和季节变化特征,非洲站的变率强于印度站,反电喷(CEJ)的发生也明显强于印度站。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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