Latitudinal Profiles of Nightside Isotropy Boundaries: Comparison of Observations and Predictions of Adaptive Magnetospheric Model

Here one can find all data for the supporting Information from the paper "Latitudinal Profiles of Nightside Isotropy Boundaries: Comparison of Observations and Predictions of Adaptive Magnetospheric Model" by V.A.Sergeev, M.V.Kubyshkina, I.V.Kubyshkin, A.Artemyev, V.Angelopoulos data.zip file contains two folders for two events studied in the paper - August 11, 2022 and August 19, 2022. Each of these two folders contains the following files for two events 1) AM03 model Fortran codes which choose tail and ring current sheet parameters (intencity and thickness), and magnetospheric tail elevation angle (based on solar wind velocity vz component) that will best fit spacecraft data (for more details see Kubyshkina et al., 2009, 2011) 2) Input data – spacecraft data in GSM (g16_gsm.dat, g17_gsm.dat, etc) SW parameters from AM02 model(params_am02.dat), initial parameters for currents and their limits (amdf.dat) 3) output data - AM03 model magnetic field for each spacecraft(am03_g16.dat, am03_g17.dat, etc) and vector of parameters (params_am03.dat) 4) output data from TA_15 (Tsyganenko and Andreeva, 2015) with modeled magnetic fields in spacecraft positions (TA15_g16.dat, TA15_g17.dat, etc)