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We present the Magnetospheric Multiscale (MMS) mission's observations of large-scale reconnection with a laminar ion exhaust containing many electron-scale filamentary current sheets, one of which exhibited a super-ion-Alfv\'enic electron jet flowing opposite to the ion exhaust jet, identified as electron-only reconnection. Despite the close proximity (a few electron inertial lengths) of the four MMS spacecraft, they recorded different electron-only reconnection signatures, including differences in the magnitude and profile of the electron jet, parallel electric fields, and dissipation jE^'+v₄, indicating extremely short-scale spatial and temporal variability. Furthermore, the leading spacecraft did not detect reconnection signatures, suggesting that MMS may have witnessed the onset of electron-only reconnection. Hall magnetic field perturbations associated with an electron-scale current sheet were detected after the onset. The dissipation jE^' in the electron-only current sheet was dominated by the component perpendicular to the magnetic field, contrasting with the dominance of the parallel component in previous large guide field reconnection events.
Pyakurel et al. (Thu,) studied this question.