TY - JOUR
T1 - Detection of Large Guide Field Electron-Only Reconnection in a Filamentary Current Sheet Immersed in a Large-Scale Magnetopause Reconnection Exhaust
AU - Pyakurel, P. S.
AU - Phan, T. D.
AU - Øieroset, M.
AU - Drake, J. F.
AU - Shay, M. A.
AU - Mallet, A.
AU - Stawarz, J.
AU - Wang, S.
AU - Oka, M.
AU - Genestreti, K. J.
AU - Ahmadi, N.
AU - Burch, J. L.
AU - Torbert, R. B.
AU - Ergun, R. E.
AU - Gershman, D. J.
AU - Giles, B. L.
AU - Strangeway, R. J.
PY - 2025/3/20
Y1 - 2025/3/20
N2 - 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-Alfvénic 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 𝐣·𝐄′≡𝐣·[𝐄+𝐯e×𝐁], 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 𝐣 ·𝐄′ 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.
AB - 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-Alfvénic 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 𝐣·𝐄′≡𝐣·[𝐄+𝐯e×𝐁], 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 𝐣 ·𝐄′ 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.
UR - http://www.scopus.com/inward/record.url?scp=105000515526&partnerID=8YFLogxK
U2 - 10.1103/physrevlett.134.115201
DO - 10.1103/physrevlett.134.115201
M3 - Article
SN - 0031-9007
VL - 134
JO - Physical Review Letters
JF - Physical Review Letters
IS - 11
M1 - 115201
ER -