TY - JOUR
T1 - Birkeland currents during substorms
T2 - Statistical evidence for intensification of Regions 1 and 2 currents after onset and a localized signature of auroral dimming
AU - Coxon, John C.
AU - Rae, I. Jonathan
AU - Forsyth, Colin
AU - Jackman, Caitriona M.
AU - Fear, Robert C.
AU - Anderson, Brian J.
N1 - Funding Information:
This work was supported by NERC joint grants NE/L007177/1 (J.C.C. and C.M.J.) and NE/L007495/1 (I.J.R. and C.F.), in addition to STFC Ernest Rutherford grant ST/L002809/1 (J.C.C. and R.C.F.).
PY - 2017/6
Y1 - 2017/6
N2 - We conduct a superposed epoch analysis of Birkeland current densities from AMPERE (Active Magnetosphere and Planetary Electrodynamics Response Experiment) using isolated substorm expansion phase onsets identified by an independently derived data set. In order to evaluate whether R1 and R2 currents contribute to the substorm current wedge, we rotate global maps of Birkeland currents into a common coordinate system centered on the magnetic local time of substorm onset. When the latitude of substorm is taken into account, it is clear that both R1 and R2 current systems play a role in substorm onset, contrary to previous studies which found that R2 current did not contribute. The latitude of substorm onset is colocated with the interface between R1 and R2 currents, allowing us to infer that R1 current closes just tailward and R2 current closes just earthward of the associated current disruption in the tail. AMPERE is the first data set to give near-instantaneous measurements of Birkeland current across the whole polar cap, and this study addresses apparent discrepancies in previous studies which have used AMPERE to examine the morphology of the substorm current wedge. Finally, we present evidence for an extremely localized reduction in current density immediately prior to substorm onset, and we interpret this as the first statistical signature of auroral dimming in Birkeland current.
AB - We conduct a superposed epoch analysis of Birkeland current densities from AMPERE (Active Magnetosphere and Planetary Electrodynamics Response Experiment) using isolated substorm expansion phase onsets identified by an independently derived data set. In order to evaluate whether R1 and R2 currents contribute to the substorm current wedge, we rotate global maps of Birkeland currents into a common coordinate system centered on the magnetic local time of substorm onset. When the latitude of substorm is taken into account, it is clear that both R1 and R2 current systems play a role in substorm onset, contrary to previous studies which found that R2 current did not contribute. The latitude of substorm onset is colocated with the interface between R1 and R2 currents, allowing us to infer that R1 current closes just tailward and R2 current closes just earthward of the associated current disruption in the tail. AMPERE is the first data set to give near-instantaneous measurements of Birkeland current across the whole polar cap, and this study addresses apparent discrepancies in previous studies which have used AMPERE to examine the morphology of the substorm current wedge. Finally, we present evidence for an extremely localized reduction in current density immediately prior to substorm onset, and we interpret this as the first statistical signature of auroral dimming in Birkeland current.
KW - AMPERE
KW - Birkeland currents
KW - magnetotail reconnection
KW - Regions 1 and 2 currents
KW - substorm current wedge
KW - substorms
UR - http://www.scopus.com/inward/record.url?scp=85021427468&partnerID=8YFLogxK
U2 - 10.1002/2017JA023967
DO - 10.1002/2017JA023967
M3 - Article
AN - SCOPUS:85021427468
SN - 2169-9380
VL - 122
SP - 6455
EP - 6468
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 6
ER -