Key points are not available for this paper at this time.
Particle‐injection events are monitored on three geosynchronous satellites to determine the occurrences of magnetospheric substorms: for every consecutive pair of substorms found, the time interval Δ t between substorm onsets is determined. In this manner, 1001 values of Δ t are obtained. A statistical analysis of the Δ t values finds that the most‐probable time between substorms onsets is Δ t ≈ 2.75 hours: this is interpreted to be the period between substorms when substorms occur cyclically. The statistical analysis of the Δ t values also finds a random probability for the occurrence of substorms with a mean time between random substorms of about 5 hours: it is speculated that this random occurrence may be caused by a property of the solar wind that varies randomly with an approximately 5‐hour time scale. About 1500 substorms occur per year: about half are periodic and about half occur randomly.
Borovsky et al. (Mon,) studied this question.