ANALYSIS OF THE DAILY HOURLY DEPARTURES OF THE GEOMAGNETIC H FIELD OVER LOW-LATITUDE STATIONS

I. Adimula, G. I. Ojerheghan
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Abstract

The telecommunication technologies deployed in the last decades have shown that there are better days ahead. From electric telegraphs systems in the 19th century to today’s wireless communication using satellites and land links (Lanzerotti, 2001). The horizontal component (H-field) of the geomagnetic field has great impacts in the present-day communication technologies. The aim of this paper was to analyse the daily hourly departures of geomagnetic H-field along the low-latitude stations on the equatorial chain in relation to their correlation coefficients with their longitudes. The magnitude of H-component is a very significant factor in the determination of the total magnetic field of any location on the earth. The baseline values (H0) which is the average of H components at 23LT, 24LT, 1LT and 2LT were subtracted from the hourly values of H (Ht) to obtain the hourly departures of H (dH). The hourly departures of H (dH) from the baseline is non-cyclic since H1 ≠ H24 as observed over the three MAGDAS stations in Nigeria. The correlation coefficients between dHs of Lagos/Ilorin, Ilorin/Abuja and Abuja/Ilorin are 0.97, 0.75 and 0.66 respectively. This suggests that substorms are deflected eastwards along different longitudes due to the rotation of the earth such that locations in the same longitudes have the same hourly departures. There is no solar radiation during the nighttime, thus dH should be zero but for the energy stored in the magnetotail, the reduction of hourly departures towards nighttime in Nigeria is evident. This is further revealed as the midnight dH amplitudes decrease regularly. The eastward motion of the electrons during substorms was suggested to be responsible for the reduction of the H-field at the nightside magnetotail region for all the stations. These findings will assist the telecommunication companies to know which location is best for their transmitters to be sited in order to reduce loss of signals along the optical cables to the receivers. Furthermore, global telecomms companies should have business continuity plan which should include risk assessment and prompt response to geomagnetic disturbances being one of the causes for telecommunication outages.
低纬度台站地磁场日逐时偏差分析
过去几十年部署的电信技术表明,未来的日子会更好。从19世纪的电报系统到今天使用卫星和陆地链路的无线通信(Lanzerotti, 2001)。地磁场的水平分量(h场)对当今的通信技术有很大的影响。本文的目的是分析赤道链上低纬度台站的h场日逐时偏离与经度的相关系数关系。在确定地球上任何位置的总磁场时,h分量的大小是一个非常重要的因素。基线值(H0)是23LT, 24LT, 1LT和2LT H分量的平均值,从H (Ht)的小时值中减去H (dH)的小时偏离。尼日利亚三个MAGDAS站观测到的H (dH)逐时偏离基线是非周期性的,因为H1≠H24。拉各斯/伊洛林、伊洛林/阿布贾和阿布贾/伊洛林的dHs相关系数分别为0.97、0.75和0.66。这表明,由于地球的自转,亚暴沿着不同的经度向东偏转,因此在相同经度的位置有相同的小时偏离。夜间没有太阳辐射,因此dH应该为零,但由于储存在磁尾中的能量,尼日利亚夜间每小时偏离的减少是明显的。这进一步揭示了午夜dH振幅有规律地下降。亚暴期间电子向东运动是所有台站夜侧磁尾区h场减小的原因。这些调查结果将有助于电信公司了解其发射机的最佳位置,以减少沿光缆传输到接收器的信号损失。此外,全球电信公司应制定业务连续性计划,其中应包括风险评估和迅速应对作为电信中断原因之一的地磁干扰。
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