J. Watermann et al., SPACE-TIME STRUCTURE OF THE MORNING AURORA INFERRED FROM COINCIDENT DMSP-F6, DMSP-F8, AND SONDRESTROM INCOHERENT-SCATTER RADAR OBSERVATIONS, Journal of atmospheric and terrestrial physics, 55(14), 1993, pp. 1729
On rare occasions, observations from the DMSP-F6 and -F8 spacecraft an
d the Sondrestrom incoherent scatter radar coincide in space. Such coi
ncidence offers a unique opportunity to study temporal vs spatial vari
ations on a small scale. We discuss data from one of those occasions,
with observations made in the dawn sector in the presence of moderate
auroral precipitation during a magnetically quiet period. The DMSP sat
ellites measured vertical electron and ion flux and cross-track plasma
drift while the radar measured the ionospheric electron density distr
ibution and line-of-sight plasma velocities. We combine these data set
s to construct a two-dimensional map of a possible auroral pattern abo
ve Sondrestrom. It is characterized by the following properties. No di
fference is seen between the gross precipitation patterns measured alo
ng the DMSP-F6 and -F8 trajectories (separated by 32 km in magnetic ea
st-west direction and some 4 s in travel time in magnetic north-south
direction), except that they are not exactly aligned with the L shells
. However, F6 and F8 observed minor differences in the small-scale str
uctures. More significant differences are found between small-scale fe
atures in the DMSP precipitation measurements and in radar observation
s of the E-region plasma density distribution. These measurements are
separated by 74 km, equivalent to 2.4-degrees, in magnetic longitude,
and 0-40 s in time along the spacecraft trajectories (varying with mag
netic latitude). Large-scale magnetospheric-ionospheric surfaces such
as plasma flow reversal, poleward boundary of the keV ion and electron
precipitation, and poleward boundary of E-region ionization, coincide
. The combined data suggest that the plasma flow reversal delineates t
he polar cap boundary, that is, the boundary between precipitation cha
racteristic for the plasma mantle and for the plasma sheet boundary la
yer.