Abstract
FAST observations of downward current regions: Effect of ionospheric constraints on parallel signatures
FAST observations of downward current regions: Effect of ionospheric constraints on parallel signatures
K.-J. Hwang
NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
K. A. Lynch
Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire, USA
D. L. Newman
Center for Integrated Plasma Studies, University of Colorado, Boulder, Colorado, USA
C. W. Carlson
Space Sciences Laboratory, University of California, Berkeley, California, USA
Downward current region auroral crossings by the FAST (Fast Auroral Snapshot) spacecraft show that divergent electric fields
which are perpendicular to the geomagnetic field (E
) have two types of structures: those whose potential contours close below the spacecraft but above the ionosphere (U-shaped),
and those that are not completely closed but partially couple to the low-altitude ionosphere (composite). Using FAST data
from above 3000 km altitude, we investigate parallel signatures of particle motions in these downward current regions, focusing
on the distinctions between U-shaped and composite potential structures. We analyze probability density functions of electron
velocity moments and ion energies, and power spectral density scaling laws of wave turbulence above the potential drop. Results
indicate that U-shaped potential structures show aspects of fully developed turbulence. Composite structures are often characterized
by intermittent signatures, possibly because of lower ionospheric constraints. These results support a picture of an evolutionary
process from composite to U-shaped potential structures in downward current regions.
Received 6
February
2008;
accepted 12
December
2008;
published 21
February
2009.
Citation: Hwang, K.-J., K. A. Lynch, D. L. Newman, and C. W. Carlson
(2009),
FAST observations of downward current regions: Effect of ionospheric constraints on parallel signatures,
J. Geophys. Res.,
114,
A02219,
doi:10.1029/2008JA013080.