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The past forty years of space research have seen a substantial improvement in our understanding of the Earth s magnetosphere and its coupling with the solar wind and interplanetary magnetic ?eld (IMF). The magnetospheric str- ture has been mapped and major processes determining this structure have been de?ned. However, the picture obtained is too often static. We know how the magnetosphere forms via the interaction of the solar wind and IMF with the Earth s magnetic ?eld. We can describe the steady state for various upstream conditions but do not really understand the dynamic processes...

The past forty years of space research have seen a substantial improvement in our understanding of the Earth s magnetosphere and its coupling with the solar wind and interplanetary magnetic ?eld (IMF). The magnetospheric str- ture has been mapped and major processes determining this structure have been de?ned. However, the picture obtained is too often static. We know how the magnetosphere forms via the interaction of the solar wind and IMF with the Earth s magnetic ?eld. We can describe the steady state for various upstream conditions but do not really understand the dynamic processes...