The list of substorms and pseudosubstorms used in the paper entitled "Differences in Ultra-Low-Frequency Waves Associated with Dipolarization in the Near-Earth Magnetotail Between Substorms and Pseudosubstorms"

Text files containing the lists of substorm and pseudosubstorm events selected for the present study, including dipolarization onset times and THEMIS spacecraft locations. From the left to right columns: the date (in the format of YYYYMMDD) and time (in the format of hh:mm:ss) of initial auroral brightening (from Fukui et al., 2020; Nishimura et al., 2011); the THEMIS all-sky imager (ASI) station where the initial auroral brightening was observed; the name of the THEMIS spacecraft located in the plasma sheet during the event; the dipolarization onset time in the format of hh:mm:ss; and the probe’s location in geocentric solar magnetospheric (GSM) coordinates (X, Y, and Z in Earth’s radius, RE) at the time of dipolarization onset, along with the radial distance R in RE. Multiple entries may appear for a single event if more than one THEMIS spacecraft observed dipolarization. Substorms and pseudosubstorms are defined as events with and without auroral poleward expansion, respectively (Fukui et al., 2020).