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. There are: (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. 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.This work has been funded by the Russian Science Foundation Grant 14-17-00072