MMS observation of asymmetric reconnection supported by 3-D electron pressure divergence
Kevin J. Genestreti, Ali Varsani, Jim L. Burch, Paul A. Cassak, Roy B., Torbert, Rumi Nakamura, Robert E. Ergun, Tai D. Phan, Sergio Toledo-Redondo,, Michael Hesse, Shan Wang, Barbara L. Giles, Chris T. Russell, Zoltan, V\"or\"os, Kyoung-Joo Kim, Jonathan P. Eastwood

TL;DR
This study uses MMS observations to analyze asymmetric magnetic reconnection at the magnetopause, highlighting the dominant role of pressure divergence in energy conversion within the electron diffusion region.
Contribution
It provides detailed measurements of the electron diffusion region, emphasizing the significance of pressure divergence over inertial effects in energy conversion during asymmetric reconnection.
Findings
Pressure divergence dominates inertial effects in energy conversion.
Both gyrotropic and agyrotropic pressures contribute to energy transfer.
Electron-scale structures are present in the out-of-plane direction during reconnection.
Abstract
We identify a dayside electron diffusion region (EDR) encountered by the Magnetospheric Multiscale (MMS) mission and estimate the terms in generalized Ohm's law that controlled energy conversion near the X-point. MMS crossed the moderate-shear (130 degrees) magnetopause southward of the exact X-point. MMS likely entered the magnetopause far from the X-point, outside the EDR, as the size of the reconnection layer was less than but comparable to the magnetosheath proton gyro-radius, and also as anisotropic gyrotropic "outflow" crescent electron distributions were observed. MMS then approached the X-point, where all four spacecraft simultaneously observed signatures of the EDR, e.g., an intense out-of-plane electron current, moderate electron agyrotropy, intense electron anisotropy, non-ideal electric fields, non-ideal energy conversion, etc. We find that the electric field associated with…
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