Outputs from the SOPHIE (Forsyth et al., 2015, 10.1002/2015JA021343) substorm onset and phase detection technique for SuperMAG data between 2000 and 2002 (inclusive).This version has been updated in to include the MLT and MLAT of the SuperMAG station providing the SML data and as well as the change of SML during the phase (DeltaSML) value of SML at the end of each phase (SMLatEnd)The files provide the start times of growth/energy input, expansion and recovery phases determined by SOPHIE for the following EPTs:2023JA031812_DS01 - EPT 052023JA031812_DS02 - EPT 102023JA031812_DS03 - EPT 152023JA031812_DS04 - EPT 202023JA031812_DS05 - EPT 252023JA031812_DS06 - EPT 302023JA031812_DS07 - EPT 352023JA031812_DS08 - EPT 402023JA031812_DS09 - EPT 452023JA031812_DS10 - EPT 502023JA031812_DS11 - EPT 552023JA031812_DS12 - EPT 602023JA031812_DS13 - EPT 652023JA031812_DS14 - EPT 702023JA031812_DS15 - EPT 752023JA031812_DS16 - EPT 802023JA031812_DS17 - EPT 852023JA031812_DS18 - EPT 902023JA031812_DS19 - EPT 95Data generated for "On the association of substorm identification methods" by Lao et al., submitted to J. Geophys. Res.The data is presented in 7 columns: -The date and time of the first data point in the given phase (YYYY/MM/DD-HH:MM:SS)The phase number (1 for growth/energy input, 2 for expansion, 3 for recovery)A flag indicating that the rate of change of SMU is similar to that of SML in the expansion phase (0 for no flag, 1 for flag)MLT of the active SML station at the shown timeMLAT of the active SML station at the shown timeThe change in SML from the start of the phase to the end of the phase (i.e. from the time given on that line to the time given on the following line)The value of SML at the end of the phase.The original SuperMAG indices can be downloaded from https://supermag.jhuapl.edu/