EGU26-22866, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-22866
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 05 May, 08:30–10:15 (CEST), Display time Tuesday, 05 May, 08:30–12:30
 
Hall X4, X4.175
Direct observation of ion-electron decoupling in magnetic reconnection 
Yong Cun Zhang, Lei Dai, and Chi Wang
Yong Cun Zhang et al.
  • State Key Laboratory of Solar Activity and Space Weather, National Space Science Center

Ion-electron decoupling at ion scale lead to Hall effect, the indicative process of collisionless magnetic reconnection. Past observations have revealed the features of Hall current system in L direction, Hall magnetic field in M direction and Hall electric field in N direction. However until now, there is no observations on the ion-electron decoupling(Hall current)in N direction, where Hall effect originates. In this study, using MMS observation, we find ion-electron decoupling(Hall current)in N direction in the separatrix region at the magnetospheric side of a reconnection current sheet. A comprehensive analysis provides the insight to the process of ion-electron decoupling, regarding electron motion, composition of Hall electron, and charge distribution. From micro mechanism, the results deep our understanding of solar wind-magnetosphere coupling triggered by reconnection, and support the upcoming study based the observation from launched SMILE mission.

How to cite: Zhang, Y. C., Dai, L., and Wang, C.: Direct observation of ion-electron decoupling in magnetic reconnection , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22866, https://doi.org/10.5194/egusphere-egu26-22866, 2026.