Abstract

AbstractWe examine how Sudden Commencements (SCs) and Storm Sudden Commencements (SSCs) influence the occurrence of high rates of change of the magnetic field (R) as a function of geomagnetic latitude. These rapid, high amplitude variations in the ground‐level geomagnetic field pose a significant risk to ground infrastructure, such as power networks, as the drivers of geomagnetically induced currents. We find that rates of change of ∼30 nT min−1 at near‐equatorial stations are up to 700 times more likely in an SC than in any random interval. This factor decreases with geomagnetic latitude such that rates of change around 30 nT min−1 are only up to 10 times more likely by 65°. At equatorial latitudes we find that 25% of all R in excess of 50 nT min−1 occurs during SCs. This percentage also decreases with geomagnetic latitude, reaching ≤1% by 55°. However, the time period from the SC to 3 days afterward accounts for ≥90% of geomagnetic field fluctuations over 50 nT min−1, up to ∼60° latitude. Above 60°, other phenomena such as isolated substorms account for the majority of large R. Furthermore, the elevated rates of change observed during and after SCs are solely due to those classified as SSCs. These results show that SSCs are the predominant risk events for large R at mid and low latitudes, but that the risk from the SC itself decreases with latitude.

Highlights

  • One of the main pathways through which Space Weather can impact society is through damage to groundbased infrastructure caused by the generation of Geomagnetically Induced Currents (GICs)

  • In this work we have assessed the contribution of Sudden Commencements (SCs) to large rates of change of the horizontal magnetic field (R), exploring this as a function of latitude and level of variability

  • Large rates of the change of the magnetic field would be expected to drive large GICs, which may pose a risk to the operation of power networks

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Summary

Introduction

One of the main pathways through which Space Weather can impact society is through damage to groundbased infrastructure caused by the generation of Geomagnetically Induced Currents (GICs). GICs originate from the induced Ground Electric Field (GEF), which itself is driven by high amplitude magnetic field fluctuations and geological conductivity gradients. GICs can be generated in any long grounded conductor, including power grids, pipelines or rail networks (Boteler et al, 1998). The impact of widespread power network failure has been estimated at billions of US dollars a day (Oughton et al, 2017, 2019). Direct measurements of GICs in infrastructure are sparse, either due to their commercial sensitivity or expense in performing the observations. Indirect observations of GICs in power lines

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