Satellite Experiments Simultaneous with Antarctic Measurements (SESAME
) is one of the four ground-based programmes within the NASA/ISAS Glob
al Geospace Science (GGS) mission, itself part of the International So
lar-Terrestrial Physics (ISTP) programme. The scientific objectives of
SESAME are carefully selected to make an invaluable contribution to t
he GGS mission by capitalising on the unique geophysical advantages of
Antarctica for geospace research. These arise mainly from the large d
isplacement of the geographic and geomagnetic poles. Specifically, SES
AME is designed to study the ionospheric effects of merging at the mag
netopause, reconnection in the geomagnetic tail and its relationship t
o substorms, mapping of significant geospace boundaries to ionospheric
altitudes, plasma wave generation and propagation at high latitudes,
and ionosphere-thermosphere interactions. The experimental programme i
s centred at Halley (76 degrees S, 27 degrees W) but also utilises aut
omatic geophysical observatories located poleward of Halley. The suite
of instruments provides an excellent image of the inner boundary of g
eospace and thus is complementary to the GGS spacecraft measurements.
The data products that will be supplied as key parameters to the GGS e
xperimenters on a routine basis are described. A brief review of previ
ous results is presented, and some of the significant scientific quest
ions to be addressed using the combination of ground-based and space-b
ased observations are discussed.