摘要：We investigate the longitudinal structure of the oxygen torus in the inner magnetosphere for a specifc event found
on 12 September 2017, using simultaneous observations from the Van Allen Probe B and Arase satellites. It is found
that Probe B observed a clear enhancement in the average plasma mass (M) up to 3–4 amu at L=3.3–3.6 and magnetic local time (MLT)=9.0 h. In the afternoon sector at MLT~16.0 h, both Probe B and Arase found no clear enhancements in M. This result suggests that the oxygen torus does not extend over all MLT but is skewed toward the dawn.
Since a similar result has been reported for another event of the oxygen torus in a previous study, a crescent-shaped
torus or a pinched torus centered around dawn may be a general feature of the O+ density enhancement in the
inner magnetosphere. We newly fnd that an electromagnetic ion cyclotron (EMIC) wave in the H+ band appeared
coincidently with the oxygen torus. From the lower cutof frequency of the EMIC wave, the ion composition of the
oxygen torus is estimated to be 80.6% H+, 3.4% He+, and 16.0% O+. According to the linearized dispersion relation for
EMIC waves, both He+ and O+ ions inhibit EMIC wave growth and the stabilizing efect is stronger for He+ than O+.
Therefore, when the H+ fraction or M is constant, the denser O+ ions are naturally accompanied by the more tenuous He+ ions, resulting in a weaker stabilizing efect (i.e., larger growth rate). From the Probe B observations, we fnd
that the growth rate becomes larger in the oxygen torus than in the adjacent regions in the plasma trough and the
plasmasphere.
