Transport of thermal‐energy ionospheric oxygen (O+) ions between the ionosphere and the plasma sheet and ring current at quiet times preceding magnetic storms

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Abstract

The presence of energetic O + ions in the ring current at the onset of a magnetic storm prompts the question of the possible role of “in‐transit” ionospheric O + ions between the ionosphere and the plasma sheet and ring current in the quiet periods immediately preceding the main phase of a magnetic storm. Thermal‐energy O + ions are often observed in the quiet time high‐altitude (>7000 km) polar ionosphere on Akebono, at temperatures of ∼0.2–0.3 eV and flow velocities of a few km/s. In this paper, we use single‐particle trajectory simulation to study the transport of these ions in the periods preceding a number of large magnetic storms (Dst < −100 nT). Our simulation shows that due to centrifugal ion acceleration at higher altitudes (above ∼3 R E altitude), about 10–20% of polar wind and other low‐energy O + ions reaches the plasma sheet during such periods; the actual percentage is a factor of ∼3 larger in the dusk sector on average compared with the dawn sector and dependent on the IMF and the O + ion temperature. This provides a low but non‐negligible flux of O + ions between the ionosphere and the plasma sheet and ring current, which is believed to constitute a significant “in‐transit” oxygen ion population over a period of a few (∼4) hours preceding a magnetic storm. Such a population could explain the presence of energetic O + ions at the onset of the main phase of the storm, when the heavy ions could potentially modify the evolution of the ring current.

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