TY - JOUR
T1 - The Impact of Sudden Commencements on Ground Magnetic Field Variability
T2 - Immediate and Delayed Consequences
AU - Smith, Andrew W.
AU - Forsyth, Colin
AU - Rae, Jonathan
AU - Rodger, Craig J.
AU - Freeman, Mervyn P.
N1 - Funding information: A. W. Smith and I. J. Rae were supported by STFC Consolidated Grant ST/S000240/1, and NERC grants NE/P017150/1 and NE/V002724/1. C. Forsyth was supported by the NERC Independent Research Fellowship NE/N014480/1, NERC grant NE/V002724/1 and STFC Consolidated Grant ST/S000240/1. C. J. Rodger was supported by the New Zealand Ministry of Business, Innovation & Employment through Endeavor Fund Research Program contract UOOX2002. M. P. Freeman was supported by NERC grants NE/P016693/1 (SWIGS) and NE/V002716/1 (SWIMMR SAGE). The analysis in this paper was performed using python, including the pandas (McKinney, 2010), numpy (Van Der Walt et al., 2011), scikit-learn (Pedregosa et al., 2011), scipy (Virtanen et al., 2020) and matplotlib (Hunter, 2007) libraries. The authors thank the involved national institutes, the INTERMAGNET network and the ISGI.
PY - 2021/7
Y1 - 2021/7
N2 - We 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.
AB - We 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.
KW - geomagnetic perturbations
KW - geomagnetically induced currents
KW - GICs
KW - interplanetary shocks
KW - sudden commencements
UR - http://www.scopus.com/inward/record.url?scp=85111657916&partnerID=8YFLogxK
U2 - 10.1029/2021sw002764
DO - 10.1029/2021sw002764
M3 - Article
SN - 1542-7390
VL - 19
SP - 1
EP - 17
JO - Space Weather
JF - Space Weather
IS - 7
M1 - e2021SW002764
ER -