We have investigated similarities and differences between substorms occurri
ng in stormtime and those in less disturbed periods, using data from the MI
CS instrument on CRRES to investigate composition changes in ring current i
ons in the energy range 70-400 keV/e. A statistical study shows that while
substorms show some size and composition dependence on Dst, the strongest e
ffect is that substorm injected energetic ion composition reflects the back
ground population at energisation.
These results are supported by a superposed epoch analysis which shows that
the composition of storm time injections is similar to the set of all (sto
rm and quiet rime) oxygen rich injections. Moreover, these injections which
have a high initial oxygen background, which is the condition that pertain
s in storms. We conclude that, during solar maximum when these measurements
were made, substorms are not directly responsible for the injection of oxy
gen ions into the ring current. (C) 1998 Elsevier Science Ltd. All rights r
eserved.