Datasets for "Recreating the Horizontal Magnetic Field at Colaba During the Carrington Event with Geospace Simulations", Blake et al. (2021), Space Weather

Sample datasets that appear in the 2021 paper "<strong><em>Recreating the Horizontal Magnetic Field at Colaba During the Carrington Event with Geospace Simulations</em></strong>", Blake et al. (2021), submitted to the AGU Space Weather Journal, DOI: TBD The complete SWMF simulation folders (including parameter and log files etc.) can be requested from NASA's Community Coordinated Modeling Center. ################################# <strong>Solar_Wind_Drivers/</strong> Both SWMF solar wind input files for Scenarios 1 and 2 referenced in the paper. These have the following columns: Year, Month, Day, Hour, Minute, Second, Milisecond, Bx(nT), By(nT), Bz(nT), Vx(km/s), Vy(km/s), Vz(km/s), n(cm^-3), T(K) <strong>#-----------------------------------------------------</strong> <strong>Digitised_Historical_Bfields/</strong> Contains digitised BH data minus baseline for: - Barnaul and St. Petersburg (taken from <em>Nevanlinna et al.</em> 2008, 10.5194/angeo-28-917-2010) - Rome (taken from <em>Blake et al.</em> 2020, 10.1029/2019JA027336) - Colaba (taken from Tsurutani et al. 2003, 10.1029/2002JA009504). These data were digitised using WebPlotDigitiser. <strong>#-----------------------------------------------------</strong> <strong>ScenarioX_Bdata.zip</strong> -Each zipped folder contains all of the SWMF calculated B-fields for the three Scenarios in the paper. Also included are log files (log* and geo*) containing calculated indices such as Dst. The times referenced are for 2019, but as described in the paper, conditions were changed to emulate 1859. <strong>#-----------------------------------------------------</strong> <strong>Scenario1_Magnetosphere3D_0630.out</strong> -Single SWMF 3D magnetosphere output file for 0630 GMT during Scenario 1. This data can be read and plotted using the pybats Python library. <strong>Scenario1_Ionosphere2D.tec</strong> -Single SWMF 2D ionosphere output for 0630 GMT during Scenario 1. <strong>#-----------------------------------------------------</strong>