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• W4296251627 abstract "Abstract Oxygen ions are a major constituent of magnetospheric plasma, yet the role of oxygen in processes such as magnetic reconnection continues to be poorly understood. Observations show that significant amounts of energized O + can be present in a magnetotail current sheet (CS). A population of thermal O + only has a relatively minor effect on magnetic reconnection. Despite this, published studies have so far only concentrated on the role of the low‐energy thermal O + . We present a study of magnetic reconnection in a thinning CS with energized O + present. Well‐established, three‐species, 2.5D particle‐in‐cell (PIC) kinetic simulations are used. Simulations of thermal H + and thermal O + validate our setup against published results. We then energize a thermal background O + based on published in situ measurements. A range of energization is applied to the background O + . We discuss the effects of energized O + on CS thinning and the onset and evolution of magnetic reconnection. The presence of energized O + causes a two‐regime onset response in a thinning CS. As energization increases in the lower‐regime, reconnection develops at a single primary X ‐line, increases time‐to‐onset, and suppresses the rate of evolution. As energization continues to increase in the higher‐regime, reconnection develops at multiple X ‐lines, forming a stochastic plasmoid chain; decreases time‐to‐onset; and enhances evolution via a plasmoid instability. Energized O + drives a depletion of the background H + around the central CS. As the energization increases, the CS thinning begins to slow and eventually reverses." @default.
• W4296251627 created "2022-09-19" @default.
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• W4296251627 date "2022-09-01" @default.
• W4296251627 modified "2023-09-26" @default.
• W4296251627 title "Energized Oxygen in the Magnetotail: Onset and Evolution of Magnetic Reconnection" @default.
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• W4296251627 doi "https://doi.org/10.1029/2020ja028381" @default.
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