The Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) mission us
es a suite of imaging instruments to investigate the global response of the
magnetosphere to changing solar wind conditions. Detailed science question
s that fall under this broad objective include plasma processes that occur
on the dayside, flanks, and nightside of the magnetosphere. The IMAGE orbit
has been carefully designed to optimize the investigation of these plasma
processes as the orbit precesses through the magnetospheric regions. We dis
cuss here the phasing of the IMAGE orbit during the two-year prime mission
and the relationship between the orbit characteristics and the critical sci
ence objectives of the mission.