Empirical modeling of the geomagnetosphere for SIR and CME-driven magnetic storms

Data associated with Journal of Geophysical Research: Space Physics article titled: "Empirical modeling of the geomagnetosphere for SIR and CME-driven magnetic storms", by V. A. Andreeva and N. A. Tsyganenko.<br> There are:<br> (1) 'Subset_{1,2,3}.dat' incorporating the spacecraft ephemerids and magnetic field measurements, used for the model fitting, as well as input solar wind parameters for the model; (2) 'Data_format.txt' describing the data format in subset files; (3) 'Model_parameters_set_{1,2,3}.par containing the model parameters, obtained during fitting; (4) 'Subroutine_model_TA15_with_Wi.for' - a set of Fortran subroutine for calculating the external magnetospheric magnetic field according to the model described in the paper. <br> Note, that '1', '2' and '3' in the file's name correspond to SIR-induced storms, storms induced by CME without a shock ahead and CME with a shock ahead. For more details please see the paper.