Ion composition of substorms during storm-time and non-storm-time periods

Physics

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Scientific paper

The oxygen to hydrogen ratio (O+/H+) is investigated for storm-time substorms (Dst=-195nT) and for substorms in absence of storms (non-storm-time substorms) (Dst>=-30nT). For this study we use CRRES particle and electric field data as well as indicators for storm (Dst) and substorm (AE) activity and the IMF Bz-component from IMP-8. Injection of particles into the inner magnetosphere during storms and substorms is consistent with enhanced convection caused by large-scale storm-time or dipolarization dawn-dusk electric fields in the near-Earth magnetotail. The strength of this convection is related to the magnitude and duration of the negative IMF Bz, which are both larger for storm-time substorms than for non-storm-time substorms. Non-storm-time substorms lead to only minor ring current enhancements at large /L-values (/L=5.0-7.0), while storm-time substorms can contribute the main ring current. During storms the ring current maximum can move in as far as /L=3 from its quiet time position at /L=4.5. Storm-time substorms have O+/H+ ratios of several 100%, whereas non-storm-time substorms show an O+/H+ ratio between 15% and 65%. The obvious composition difference between storm-time and non-storm-time substorms indicates that during storms one or a combination of the following factors play a role: (1) oxygen ions are preferentially accelerated/transported in the plasma sheet, (2) pre-storm conditions lead to a large reservoir of oxygen ions tailward of the oxygen trapping boundary, or (3) polar ionospheric outflow is enhanced leading to an increased convection source of oxygen ions.

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