AGU Fall Meeting, San Francisco, 6-10 December 1998
Abstract:
The German Equator-S satellite observed, between December 1997 and March
1998, a large number (more than 100) magnetopause crossings in the
low-latitude morning sector of the magnetosphere. The apogee of the
spacecraft at 67,000 km allowed the observation of magnetopause crossings
for medium to high pressure solar wind conditions. We review briefly the
magnetopause locations observed by Equator-S and relate them to solar wind
and geomagnetic conditions, as well as to geomagnetic field models. Close
to several of the crossings, intense mirror-mode structures were observed.
The orbit of Equator-S was particularly advantageous for such observations
as it remained at a nearly constant radial distance for significant periods
near apogee. Spectral analysis of the mirror-mode structures shows a
characteristic shape of a well defined shoulder at about 0.05 Hz. The main
features of the spectrum appear to be stable, despite significant changes
in the temporal distribution and shape of the structures. We discuss the
occurrence and characteristics of the observed mirror-mode episodes in
relationship with the location and nature of the magnetopause crossings
associated with them.