“…Comparison with case studies, demonstrating density (and dynamic pressure) acting on substorm activity, is hard to perform, since it is impossible in each particular case to distinguish between the triggering effect, changing merely time history of an event, and modification of the event energetics, which is of interest for our study. Petrukovich and Rusanov (2005) with the same procedure also checked the influence of some other solar wind characteristics. The effect of Mach numbers, solar wind temperature, b, IMF B x was negligible.…”