The EDR inflow region of a reconnecting current sheet in the geomagnetic tail

Author:

Burch J. L.1ORCID,Hesse M.2,Webster J. M.3,Genestreti K. J.4ORCID,Torbert R. B.45,Denton R. E.6,Ergun R. E.7,Giles B. L.8,Gershman D. J.8ORCID,Russell C. T.9,Wang S.10,Chen L.-J.8,Dokgo K.1ORCID,Hwang K.-J.1,Pollock C. J.11ORCID

Affiliation:

1. Southwest Research Institute, San Antonio, Texas 78238, USA

2. NASA Ames Research Center, Moffett Field, California 94035, USA

3. Rice University, Houston, Texas 77005, USA

4. Southwest Research Institute, Durham, New Hampshire 03824, USA

5. University of New Hampshire, Durham, New Hampshire 03824, USA

6. Dartmouth College, Hanover, New Hampshire 03755, USA

7. LASP, University of Colorado, Boulder, Colorado 80303, USA

8. NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA

9. University of California, Los Angeles, California 90095, USA

10. University of Maryland, College Park, Maryland 20742, USA

11. Denali Scientific, Fairbanks, Alaska 99743, USA

Abstract

On 6 July 2017, the four Magnetospheric Multiscale spacecrafts were positioned within an electron diffusion region (EDR) just northward of a reconnection X line. The EDR was identified by electron crescent distributions, out-of-plane current, and energy conversion. From this position, the three spacecrafts closest to the X line (within about three electron inertial lengths) were able to accurately measure the reconnection electric field and the electron inflow velocity. The reconnection rates derived from the electric field and inflow velocity measurements agree with theoretical estimates (0.11–0.17) and a previous measurement of EM in a tail reconnection event on 11 July 2017.

Funder

Goddard Space Flight Center

Publisher

AIP Publishing

Subject

Condensed Matter Physics

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