“…In this study, we focused on the most intense geomagnetic storms of solar cycle 24 (Table 1 and Figure 2), whose origin were coronal mass ejections (e.g., Watari,
2017). To characterize the magnitude of GICs computed for a given storm, we chose the standard deviation statistic, SD(GIC), as this represents the level of GIC activity during the whole storm duration (see also Alves Ribeiro et al.,
2021):
with N the number of 1‐min values and
the average value in the storm time interval. This choice, instead of GIC peak values, is due to the fact that the latter can be erroneously identified from outliers and also because GIC peak values are not necessarily simultaneous over the whole power grid (Girgis et al.,
2020).…”