- 1State Key Laboratory of Solar Activity and Space Weather, National Space Science Center,
- 2College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China
- 3Southwest Research Institute, San Antonio, TX, USA
- 4European Space Research and Technology Centre, European Space Agency (ESA), Noordwijk, The Netherlands
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.
How to cite: Anxin, Z., Duan, S., Dai, L., Hou, Y., Ren, Y., Wang, C., Fuselier, S., Escoubet, P., and Burch, J.: Observations of the magnetopause reconnection ion diffusion region with high-density O+ ions during the May 2024 superstorm, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22874, https://doi.org/10.5194/egusphere-egu26-22874, 2026.