- 1Institute of Space Physics and Applied Technology, Peking University, Beijing, China
- 2CAS Key Lab of Geospace Environment, University of Science and Technology of China, Hefei, China
- 3Space Sciences Laboratory, University of California, Berkeley, Berkeley, USA
- 4State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau, China
- 5Institut de Recherche en Astrophysique et Planetologie, CNES-CNRS-Universite Toulouse III Paul Sabatier, Toulouse, France
The recently discovered electron-only reconnection has drawn great interests due to abnormal features like lack of ion outflows and high reconnection rates. Using particle-in-cell simulations, we investigate their physical mechanisms. The reconnection rate, when normalized by ion parameters (Ri), may appear anomalously high, whereas that normalized by electron parameters (Re) remains ~0.1. We propose that the essence of high is insufficient field line bending outside the electron diffusion region, indicating an incomplete development of the ion diffusion region. It may result from bursty reconnection in thin current sheets, or small system sizes. The ion outflow diminishes at high when the gyroradius (ρi) exceeds the system size. Low-velocity ions still experience notable acceleration from Hall fields. However, a local distribution includes many high-velocity ions that experience random accelerations from different electric fields across , resulting in near-zero bulk velocities. Our study helps understand reconnection structures and the underlying physics for transitions between different regimes.
How to cite: Wang, S., Fan, C.-Y., Zhou, X.-Z., Lu, S., Lu, Q.-M., Pyakure, P., Zong, Q.-G., and Liu, Z.-Y.: New Insights on the High Reconnection Rate and the Diminishment of Ion Outflow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3165, https://doi.org/10.5194/egusphere-egu25-3165, 2025.