Orr L, Chapman S C, Gjerloev J W, Guo W
Centre for Fusion, Space and Astrophysics, University of Warwick, Coventry, UK.
Applied Physics Laboratory-John Hopkins University, Laurel, MD, USA.
Nat Commun. 2021 Mar 23;12(1):1842. doi: 10.1038/s41467-021-22112-4.
Geomagnetic substorms are a global magnetospheric reconfiguration, during which energy is abruptly transported to the ionosphere. Central to this are the auroral electrojets, large-scale ionospheric currents that are part of a larger three-dimensional system, the substorm current wedge. Many, often conflicting, magnetospheric reconfiguration scenarios have been proposed to describe the substorm current wedge evolution and structure. SuperMAG is a worldwide collaboration providing easy access to ground based magnetometer data. Here we show application of techniques from network science to analyze data from 137 SuperMAG ground-based magnetometers. We calculate a time-varying directed network and perform community detection on the network, identifying locally dense groups of connections. Analysis of 41 substorms exhibit robust structural change from many small, uncorrelated current systems before substorm onset, to a large spatially-extended coherent system, approximately 10 minutes after onset. We interpret this as strong indication that the auroral electrojet system during substorm expansions is inherently a large-scale phenomenon and is not solely due to many meso-scale wedgelets.
地磁亚暴是一种全球磁层重构现象,在此期间能量会突然传输到电离层。其核心是极光电集流,它是大规模电离层电流,是更大的三维系统——亚暴电流楔的一部分。人们提出了许多常常相互矛盾的磁层重构模型来描述亚暴电流楔的演化和结构。超级磁暴网络(SuperMAG)是一项全球合作项目,可方便地获取地面磁力仪数据。在此我们展示了运用网络科学技术来分析来自137个SuperMAG地面磁力仪的数据。我们计算了一个随时间变化的有向网络,并对该网络进行社区检测,识别出局部密集的连接组。对41次亚暴的分析表明,在亚暴开始前,由许多小的、不相关的电流系统组成,而在亚暴开始后约10分钟,会转变为一个大的空间扩展相干系统,结构发生了显著变化。我们将此解释为一个有力的迹象,表明亚暴扩展期间的极光电集流系统本质上是一种大规模现象,并非仅仅由许多中尺度的小电流楔造成。