Time Evolution of the Substorm Current Wedge from Ground and Space-based Magnetic Fields
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Date
2007-10-05Author
Connors, Martin
Russell, Christopher T.
Donovan, Eric F.
Angelopoulos, Vassilis
Mende, Stephen B.
Glassmeier, Karl-Heinz
Hayashi, Kanji
Spanswick, Emma
McFadden, James
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Over the past several years, intensive efforts have resulted in a significant
improvement in the ground instrumentation for auroral studies in North America. A
major part of this is due to the THEMIS ground program, both in the U.S. and in Canada.
The THEMIS Ground-Based Observatory network has fielded 10 additional
magnetometers in Canada and Alaska. Further THEMIS magnetometers are part of the
GEONS outreach effort, found in the continental U.S. and Alaska. Athabasca University
initiatives and collaborations have made yet further magnetometer data available, most
notably from a new network of instruments in central Alberta. Several stations of the
University of Tokyo STEP network remain operational, and some have been upgraded.
There is finally a dense enough set of magnetic data that techniques based on forward
modeling, and most relevant to the opportunity afforded by THEMIS, Automated
Regional Modeling (ARM), can be reliably used. These techniques specify where net
field-aligned current (FAC) and ionospheric electric current flow are located. In some
cases the Pedersen system can also be included based on data. Even when it is not, it can
be considered collocated with electrojet locations given by ARM. The extension into
space of the FAC (net or Pedersen) allows comparison with the perturbations observed at
THEMIS. We present results from an event on March 13, 2007, during which THEMIS
in its early orbital configuration was over central North America, clear weather prevailed,
and a substorm took place whose perturbations were ideally suited for inversion using
ARM. At about 5 UT, activations were detected from the ground with magnetic
perturbations also detected from THEMIS above the affected stations. The ground
perturbations are very well represented by a three-dimensional substorm current wedge
(SCW) system, and perturbations in space indicate radial propagation at a time when the
electrojet was expanding poleward. Little longitudinal propagation of the SCW is
suggested by the ground data.