Pc. Anderson et al., Global storm time auroral X-ray morphology and timing and comparison with UV measurements, J GEO R-S P, 105(A7), 2000, pp. 15757-15777
The Polar Ionospheric X-ray Imaging Experiment (PIXIE) on. NASA's Polar spa
cecraft provides the first global images of the amoral oval in X-rays and a
llows very accurate measurements of the timing of geomagnetic disturbances
to a degree of temporal resolution not available from previous imagers due
to its photon counting characteristics. On October 19, 1998, a magnetic clo
ud associated with a CME encountered the Earth's magnetopause near 0500 UT,
generating a magnetic storm that reached a minimum value in Dst of -139 nT
. The z component of the interplanetary magnetic field (IMF) (B-z) remained
remarkably steady for the first 10 hours of the storm as did the solar win
d particle pressure. The PIXIE and UVI instruments on the Polar spacecraft
were both imaging the auroral oval from 0800 to 1800 UT; six distinct impul
sive auroral enhancements were observed by the imagers during this time per
iod. Global imaging combined with geosynchronous particle observations allo
wed classification of the geomagnetic disturbances associated with the even
ts. Only two of the events were classified as substorms;one was classified
as a poleward boundary intensification, one was a convection bay, and one w
as a pseudobreakup. A sixth event occurred after a dramatic northward turni
ng of the IMF at the end of the 10-hour B-z south period but was very weak
and transient. The effects of the northward turning were counteracted by a
simultaneous increase in the B-y component of the IMF. The first sign of si
gnificant substorm activity occurred over 8 hours after the cloud encounter
ed the Earth and was not associated with any change in the solar wind magne
tic field or particle pressure. The cross polar cap potential remained larg
e (> 100 kV), and most of the X-ray emissions observed were associated with
enhanced earthward convection caused by large cross-tail electric fields;
50% were collected from the 0000 - 0600 magnetic local time (MLT) sector.