“…These methods have included statistical techniques (e.g., Shore et al, 2017;Weigel et al, 2002;Weimer, 2013), global scale physics-based (Magneto-HydroDynamic, MHD) models (e.g., Pulkkinen et al, 2011Pulkkinen et al, , 2013Tõth et al, 2014;Welling, 2019), machine learning-based techniques (e.g., Blandin et al, 2022;Gleisner & Lundstedt, 2001;Keesee et al, 2020;Pinto et al, 2022;Smith, Forsyth, Rae, Garton, et al, 2021;Upendran et al, 2022;Wintoft et al, 2015Wintoft et al, , 2017, or combinations of these methods (e.g., Camporeale et al, 2020). The forecast geomagnetic (or geoelectric) field predictions can then be used to drive models based on the local geology and properties of the power network to indirectly obtain GIC estimates (Beggan et al, 2013;Blake et al, 2016Blake et al, , 2018Dimmock et al, 2021;Divett et al, 2018Divett et al, , 2020Grawe & Makela, 2021;Mac Manus et al, 2022). Each model that is used to forecast the geomagnetic consequences of space weather will use the input solar wind data in a distinct fashion, and therefore may be impacted differently by the ways in which the NRT and scientific data differ.…”