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Observations of the magnetopause reconnection ion diffusion region with high-density O+ ions during the May 2024 superstorm
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Based on high-resolution measurements from NASA’s Magnetospheric Multiscale mission (MMS), we present the first direct observation of an ion diffusion region (IDR) with high number density O+ ions within the dayside magnetopause reconnection during the May 2024 superstorm. The O⁺ ion density reaches a high value of ~3.3 cm⁻³. It helps study heavy-ion dynamics in dayside magnetopause reconnection. In the vicinity of IDR, O⁺ ions exhibit distinct acceleration to 300 km/s along the normal direction caused by the enhanced Hall electric field (ENmax≈ 80 mV/m). The distorted ion velocity distributions reveal the complex energization processes in the ion diffusion region. Crucially, these O⁺ ion dynamics can reduce the reconnection rate by ~ 25.3%, providing the result that heavy-ion dominance alters magnetopause reconnection physics during the superstorm. This study advances our understanding of magnetopause reconnection by demonstrating that storm-enhanced O⁺ populations modify the structure of diffusion regions, particle energization, and the reconnection rate.
Title: Observations of the magnetopause reconnection ion diffusion region with high-density O+ ions during the May 2024 superstorm
Description:
Based on high-resolution measurements from NASA’s Magnetospheric Multiscale mission (MMS), we present the first direct observation of an ion diffusion region (IDR) with high number density O+ ions within the dayside magnetopause reconnection during the May 2024 superstorm.
The O⁺ ion density reaches a high value of ~3.
3 cm⁻³.
It helps study heavy-ion dynamics in dayside magnetopause reconnection.
In the vicinity of IDR, O⁺ ions exhibit distinct acceleration to 300 km/s along the normal direction caused by the enhanced Hall electric field (ENmax≈ 80 mV/m).
The distorted ion velocity distributions reveal the complex energization processes in the ion diffusion region.
Crucially, these O⁺ ion dynamics can reduce the reconnection rate by ~ 25.
3%, providing the result that heavy-ion dominance alters magnetopause reconnection physics during the superstorm.
This study advances our understanding of magnetopause reconnection by demonstrating that storm-enhanced O⁺ populations modify the structure of diffusion regions, particle energization, and the reconnection rate.
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