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Buchbeschreibung Zustand: New. pp. xiv + 328. Bestandsnummer des Verkäufers 26291561
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Buchbeschreibung PF. Zustand: New. Bestandsnummer des Verkäufers 6666-IUK-9781402027673
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Buchbeschreibung Soft Cover. Zustand: new. This item is printed on demand. Bestandsnummer des Verkäufers 9781402027673
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Buchbeschreibung Zustand: New. pp. xiv + 328. Bestandsnummer des Verkäufers 7589174
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Buchbeschreibung Taschenbuch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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 with many time constants ranging from fractions of a second to days and the system rarely attains a steady state. Two decades ago, it became clear that further progress would require multi-point measurements. Since then, two multi-spacecraft missions have been launched - INTERBALL in 1995/96 and CLUSTER II in 2000. The objectives of these missions d- fered but were complementary: While CLUSTER is adapted to meso-scale processes, INTERBALL observed larger spatial and temporal scales. However, the number of papers taking advantage of both missions simul- neously is rather small. 344 pp. Englisch. Bestandsnummer des Verkäufers 9781402027673
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Buchbeschreibung Kartoniert / Broschiert. Zustand: New. Bestandsnummer des Verkäufers 458473933
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Buchbeschreibung Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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 with many time constants ranging from fractions of a second to days and the system rarely attains a steady state. Two decades ago, it became clear that further progress would require multi-point measurements. Since then, two multi-spacecraft missions have been launched - INTERBALL in 1995/96 and CLUSTER II in 2000. The objectives of these missions d- fered but were complementary: While CLUSTER is adapted to meso-scale processes, INTERBALL observed larger spatial and temporal scales. However, the number of papers taking advantage of both missions simul- neously is rather small. Bestandsnummer des Verkäufers 9781402027673
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Buchbeschreibung Zustand: New. Buy with confidence! Book is in new, never-used condition 1.23. Bestandsnummer des Verkäufers bk1402027672xvz189zvxnew
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Buchbeschreibung Paperback. Zustand: Brand New. paperback/cd-rom edition. 328 pages. 9.00x6.25x0.75 inches. In Stock. Bestandsnummer des Verkäufers x-1402027672
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Buchbeschreibung Paperback / softback. Zustand: New. This item is printed on demand. New copy - Usually dispatched within 5-9 working days. Bestandsnummer des Verkäufers C9781402027673
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