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Multiscale Processes in the Earth's Magnetosphere: From Interball to Cluster: Proceedings of the NATO ARW on Multiscale Processes in the Earth's Magnetosphere: ... Physics and Chemistry Book 178)

معرفی کتاب «Multiscale Processes in the Earth's Magnetosphere: From Interball to Cluster: Proceedings of the NATO ARW on Multiscale Processes in the Earth's Magnetosphere: ... Physics and Chemistry Book 178)» نوشتهٔ Jean-André Sauvaud, Zdeněk Němeček, Zdeněk Němeček (Professor.)، منتشرشده توسط نشر Kluwer Academic Publishers در سال 2004. این کتاب در فرمت pdf، زبان انگلیسی ارائه شده است.

The book is devoted to the achievements of two complementary multispacecraft missions – INTERBALL and CLUSTER II. The advantages of these powerful instruments for magnetospheric investigations are clearly shown together with problems that were or should be overcome in the mission management and data processing and interpretation. The main goal of both missions is the investigation of coupling among different magnetospheric regions and, consequently, the core of the book deals with this topic. Nevertheless, various coupling processes are influenced by upstream conditions or triggered by solar wind or interplanetary magnetic field disturbances. The book also stresses the importance of the solar wind input on magnetospheric processes. The Editors of the book hope that it will be useful for scientists involved in Solar– Terrestrial relations or Space Weather programs as well as for students of space or plasma physics. The book surveys present knowledge and puts it into context of the latest results of aforementioned missions. Since the book treats not only achievements but the problems of multispacecraft observations as well, it can serve as a tool for the planning of further missions. Contents......Page 8 Dedication......Page 6 Contributing Authors......Page 10 Preface......Page 14 Propagation and Evolution of ICMEs in the Solar Wind......Page 16 The Solar Wind Interaction with Planetary Magnetospheres......Page 30 An Overview of New Concepts Deduced from INTERBALL Solar Wind Investigations......Page 52 Interplanetary Discontinuities and Shocks in the Earth's Magnetosheath......Page 72 Magnetosheath Investigations: INTERBALL Contribution to the Topic......Page 88 Pressure Pulses and Cavity Mode Resonances......Page 110 Two-Point INTERBALL Observations of the LLBL......Page 126 CLUSTER: New Measurements of Plasma Structures in 3D......Page 146 Cusp Properties for By Dominant IMF......Page 164 CEP as a Source of Upstream Energetic Ions......Page 190 Magnetic Cloud and Magnetosphere—Ionosphere Response to the 6 November 1997 CME......Page 210 Multipoint Observations of Transient Event Motion Through the Ionosphere and Magnetosphere......Page 220 A Model for the MHD Turbulence in the Earth’S Plasma Sheet: Building Computer Simulations......Page 232 Cold Ionospheric Ions in the External Dayside Magnetosphere......Page 270 Role of Electrostatic Effects in Thin Current Sheets......Page 290 Bursty Bulk Flows and Their Ionospheric Footprints......Page 304 Multi-point CLUSTER Observations of VLF Risers, Fallers and Hooks at and Near the Plasmapause......Page 322 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.

the Book Is Devoted To The Achievements Of Two Complementary Multispacecraft Missions—interball And Cluster Ii. The Advantages Of These Powerful Instruments For Magnetospheric Investigations Are Clearly Shown Together With Problems That Were Or Should Be Overcome In The Mission Management And Data Processing And Interpretation.

the Main Goal Of Both Missions Is The Investigation Of Coupling Among Different Magnetospheric Regions And, Consequently, The Core Of The Book Deals With This Topic. Nevertheless, Various Coupling Processes Are Influenced By Upstream Conditions Or Triggered By Solar Wind Or Interplanetary Magnetic Field Disturbances. The Book Also Stresses The Importance Of The Solar Wind Input On Magnetospheric Processes.

the Editors Of The Book Hope That It Will Be Useful For Scientists Involved In Solar- Terrestrial Relations Or Space Weather Programs As Well As For Students Of Space Or Plasma Physics. The Book Surveys Present Knowledge And Puts It Into Context Of The Latest Results Of Aforementioned Missions. Since The Book Treats Not Only Achievements But The Problems Of Multispacecraft Observations As Well, It Can Serve As A Tool For The Planning Of Further Missions.

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