地磁风暴及其对埃塞俄比亚电网的影响

IF 0.2 Q4 ASTRONOMY & ASTROPHYSICS
G. Abraha, T. Yemane, Tsegaye Kassa
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引用次数: 0

摘要

在目前的工作中,我们分析了2015/2016年的8次地磁风暴事件,并研究了这些事件对埃塞俄比亚电网可能产生的影响。结果表明,大部分强制停电发生在事件主期和地磁风暴恢复期。这些地磁风暴在特定日期的扰动风暴时间(Dst)值、日冕物质抛射(CME)速度、太阳风速度(vsw)和行星际磁场(IMF-Bz)等指标和参数具有不同的特征。大多数观测到的地磁风暴都是由cme驱动的磁暴产生的,它们在主磁暴之前出现了风暴突然开始(SSCs),并且恢复周期也很短。太阳风速度和IMF-Bz的突然跳跃也与日冕物质抛射的发生一致。此外,这种影响还可以在地磁风暴和平静日期间的地球磁场变化中追踪到。观测到的cme驱动的风暴可以在变压器上产生高度可变的磁场,并提供强制停电,然而研究的停电并没有被认为是由地磁风暴驱动的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Geomagnetic storms and their impacts on Ethiopian power grid
In present work we analysed eight geomagnetic storm events in 2015/2016 and studied the possible influence of these events on Ethiopian power grids. The results showed that the majority of the forced power outages occurred in the period of the main phase of events and the recovery period of the geomagnetic storms. The geomagnetic storms are characterised by different indices and parameters such as the disturbance storm time (Dst) values, coronal mass ejection (CME) speed, solar wind speed (V sw) and interplanetary magnetic field (IMF-Bz) on the selected dates. In most cases the observed geomagnetic storms were produced by the CME-driven storms as they show a storm sudden commencement (SSCs) before the main storms, and also have the short recovery periods. The sudden jumps of the solar wind velocities and IMF-Bz are also consistent with occurrence of the CMEs. Moreover, this effect can be traced in changes of Earth magnetic field during geomagnetic storm and quiet days. The observed CME-driven storms can produce highly variable magnetic fields on the transformers and provide forced outages, however the studied outages have not been recognised as those one driven by a geomagnetic storm.
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来源期刊
Advances in Astronomy and Space Physics
Advances in Astronomy and Space Physics ASTRONOMY & ASTROPHYSICS-
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