In this section
@article{Mistry:2016:10.1103/PhysRevLett.117.185102,
author = {Mistry, R and Eastwood, JP and Haggerty, CC and Shay, MA and Phan, TD and Hietala, H and Cassak, PA},
doi = {10.1103/PhysRevLett.117.185102},
journal = {Physical Review Letters},
title = {Observations of Hall reconnection physics far downstream of the X-line},
url = {http://dx.doi.org/10.1103/PhysRevLett.117.185102},
volume = {117},
year = {2016}
}
TY - JOUR
AB - 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.
AU - Mistry,R
AU - Eastwood,JP
AU - Haggerty,CC
AU - Shay,MA
AU - Phan,TD
AU - Hietala,H
AU - Cassak,PA
DO - 10.1103/PhysRevLett.117.185102
PY - 2016///
SN - 1079-7114
TI - Observations of Hall reconnection physics far downstream of the X-line
T2 - Physical Review Letters
UR - http://dx.doi.org/10.1103/PhysRevLett.117.185102
UR - http://hdl.handle.net/10044/1/40716
VL - 117
ER -