五次地磁暴期间大 dB/dt 与场对齐电流之间的关系

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2024-07-03 DOI:10.1029/2024JA032483
A. L. Fleetham, S. E. Milan, S. M. Imber, G. E. Bower, J. Gjerloev, S. K. Vines
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引用次数: 0

摘要

众所周知,在地磁活动增加期间,地面磁层内的扰动会通过当地磁场随时间的快速变化(dB/dt)在地球表面的导电材料内诱发电流。这些电流被称为地磁感应电流,对地面基础设施具有潜在的有害影响。在这项研究中,我们对五次地磁暴进行了案例研究,分析了总共 19 天的 1 秒超级磁导管数据,以便更好地了解磁局部时间(MLT)的分布、dB/dt 的大小和 "尖峰 "的出现,在这些时间间隔内发现了 131,447 个超过 5 nT/s 的 dB/dt 尖峰。这些尖峰集中在三个分贝/秒区段:两个先前确定的午夜前和黎明区域热点,以及第三个以 12 分贝/秒(正午)为中心的密度较低的群体。观测到的正午尖峰集群与压力脉冲影响有关,但由于磁强计站覆盖范围不完整,并非所有调查风暴都观测到这一集群。在这三个 "热点 "位置,以 dB/dt 为单位的尖峰幅度最大。然后将这些尖峰现象与活动磁层行星电动响应实验提供的场对准电流(FAC)数据进行比较。尖峰最有可能与向上的场对准电流(56%)而不是向下的场对准电流(30%)或无场对准电流(14%)同时出现。
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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The Relationship Between Large dB/dt and Field-Aligned Currents During Five Geomagnetic Storms

During periods of increased geomagnetic activity, perturbations within the terrestrial magnetosphere are known to induce currents within conducting materials, at the surface of Earth through rapid changes in the local magnetic field over time (dB/dt). These currents are known as geomagnetically induced currents and have potentially detrimental effects on ground based infrastructure. In this study we undertake case studies of five geomagnetic storms, analyzing a total of 19 days of 1-s SuperMAG data in order to better understand the magnetic local time (MLT) distribution, size, and occurrence of “spikes” in dB/dt, with 131,447 spikes in dB/dt exceeding 5 nT/s identified during these intervals. These spikes were concentrated in clusters over three MLT sectors: two previously identified pre-midnight and dawn region hot-spots, and a third, lower-density population centered around 12 MLT (noon). The noon spike cluster was observed to be associated with pressure pulse impacts, however, due to incomplete magnetometer station coverage, this population is not observed for all investigated storms. The magnitude of spikes in dB/dt are determined to be greatest within these three “hot-spot” locations. These spike occurrences were then compared with field-aligned current (FAC) data, provided by the Active Magnetospheric Planetary Electrodynamic Response Experiment. Spikes are most likely to be co-located with upward FACs (56%) rather than downward FACs (30%) or no FACs (14%).

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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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