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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 leading from one state to another. The main dif?culty is that the magnetosphere is a comp- cated system...
Cluster was one of the two missions - the other being the Solar and Heliospheric Observatory (SOHO) - constituting the Solar Terrestrial Science Programme (STSP), the first `cornerstone' of ESA's Horizon 2000 Programme. After the catastrophic Ariane-5 accident on 4 June 1996 which destroyed the four Cluster spacecraft, the European Space Agency Science Programme Committee gave approval to refurbish the spare Cluster spacecraft and make it ready for flight. This new spacecraft, considered to be the first of a new fleet, is called Phoenix. In the meantime various options to repeat the Cluster four-point measurements are being studied. Since Phoenix, as the fifth Cluster spacecraft, will be equipped with the spare Cluster experiments, the instrumentation articles in this book are still appropriate to the new mission. Furthermore, the objectives of the recovery mission, the ground systems, the ground observation program and the theory and modelling efforts all remain unchanged. Thus this series of articles will continue to be essential to the Cluster community and to the general scientific community as the recovery mission is implemented.
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Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 133. We imagine the reader of this preface standing at the AGU bookstall wondering if the tome in hand is worth buying. The answer is “no”, except for certain trifling exceptions. Those who wish to learn about the exciting pioneering years of LLBL research should buy the book for Tim Eastman's excellent historical review, our opening chapter. When did the term “LLBL” first enter the field? Eastman will tell you, and much else besides.
Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 97. The exciting new results of CRRES and SAMPEX show that there are additional physical sources of energetic electrons and ions trapped in the Van Allen belts, some of which were completely unexpected. The NASA and Russian empirical models of the radiation belts need to be updated and extended. To outline different ways to achieve this task and to identify the less well known aspects of physical and empirical models of the radiation belts were the objectives of a workshop held in Brussels, October 17-20, 1995, entitled "Radiation Belts: Models and Standards." It was attended by over 60 delegates from all major laboratories involved in developing new physical as well as empirical models of the energy and spatial distributions of energetic electrons and ions trapped in the geomagnetic field.
Future perspectives on space-borne/ground-based state-of-the-art scientific instruments, exploration space missions, and advanced modeling/simulation methods, are intensively discussed from multilateral viewpoints regarding solar-terrestrial physics, space plasma, upper atmospheric observations for the Earth and planets. In addition to innovative technologies, international collaborations have been getting more essential and crucial factors in the space observations/missions. The novel concept, strategy, and promotion in these international collaborations are also main subjects of this conference.