In this study we examine observations made by AMPTE/CCE of energetic i
on bursts during seven substorm periods when the satellite was located
near the neutral sheet, and CCE observed the disruption cross-tail cu
rrent in situ. We compare ion observations to analytic calculations of
particle acceleration. We find that the acceleration region size, whi
ch we assume to be essentially the current disruption region, to be on
the order of 1 R(E). Events exhibiting weak acceleration had either r
elatively small acceleration regions (apparently associated with pseud
obreakup activity on the ground) or relatively small changes in the lo
cal magnetic field (suggesting that the magnitude of the local current
disruption was limited). These results add additional support for the
view that the particle bursts observed during turbulent current sheet
disruptions are due to inductive acceleration of ions.