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Observations of Hall Reconnection Physics Far Downstream of the X Line
Journal article   Open access   Peer reviewed

Observations of Hall Reconnection Physics Far Downstream of the X Line

R. Mistry, J. P. Eastwood, C. C. Haggerty, M. A. Shay, T. D. Phan, H. Hietala, P. A. Cassak and Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
Physical review letters, Vol.117(18), p.185102
10/28/2016
DOI: 10.1103/PhysRevLett.117.185102
PMID: 27835012
url
https://doi.org/10.1103/PhysRevLett.117.185102View
Published (Version of record) Open Access

Abstract

Observations made using the Wind spacecraft of Hall magnetic fields in solar wind reconnection exhausts are presented. These observations are consistent with the generation of Hall fields by a narrow ion inertial scale current layer near the separatrix, which is confirmed with an appropriately scaled particle-in-cell simulation that shows excellent agreement with observations. The Hall fields are observed thousands of ion inertial lengths downstream from the reconnection X line, indicating that narrow regions of kinetic dynamics can persist extremely far downstream.
Physical Sciences Physics Physics, Multidisciplinary Science & Technology

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