Corotating Interaction Regions: Proceedings Of An Issi Workshop 6-13 June 1998, Bern, Switzerland (space Sciences Series Of Issi)
معرفی کتاب «Corotating Interaction Regions: Proceedings Of An Issi Workshop 6-13 June 1998, Bern, Switzerland (space Sciences Series Of Issi)» نوشتهٔ A. Balogh, J. T. Gosling, J. R. Jokipii, R. Kallenbach, H. Kunow (auth.), A. Balogh, J. T. Gosling, J. R. Jokipii, R. Kallenbach, H. Kunow (eds.)، منتشرشده توسط نشر Springer Netherlands : Imprint : Springer در سال 1999. این کتاب در فرمت pdf، زبان انگلیسی ارائه شده است.
A Corotating Interaction Region (CIR) is the result of the interaction of fast solar wind with slower solar wind ahead. CIRs have a very large three-dimensional ex tent and are the dominant large-scale structure in the heliosphere on the declining and minimum phase of the solar activity cycle. Until recently, however, CIRs could only be observed close to the ecliptic plane, and their three-dimensional structure was therefore not obvious to observers and theoreticians alike. Ulysses was the first spacecraft allowing direct exploration of the third dimen sion of the heliosphere. Since 1992, when it has entered a polar orbit that takes it 0 up to 80 latitude, the spacecraft's performance has been flawless and the mission has provided excellent data from a superbly matched set of instruments. Perhaps the most exciting observation during Ulysses' first passage towards the south pole of the Sun was a strong and long lasting CIR whose energetic particle effects were observed up to unexpectedly high latitudes. These observations, documented in a number of publications, stimulated considerable new theoretical work. This Volume Gives A Comprehensive And Integrated Overview Of Current Knowledge And Understanding Of Corotating Interaction Regions (cirs) In The Solar Wind. It Is The Result Of A Workshop At Issi, Where Space Scientists Involved In The Ulysses, Pioneer, Voyager, Imp-8, Wind, And Soho Missions Exchanged Their Data And Interpretations With Theorists In The Fields Of Solar And Heliospheric Physics. The Book Provides A Broad Synthesis Of Current Understanding Of Cirs, Which Form At The Interface Between The Fast Solar Wind Originating In The Northern And Southern Coronal Holes And The Slow Solar Wind That Originates Near And Within Coronal Streamers Surrounding The Heliomagnetic Equator. Cirs Are The Dominant Structure In The Heliosphere Near And Beyond Earth On The Declining Phase And Near The Minimum Of The 11-year Solar Activity Cycle. Particles Energized At The Shocks That Bound Cirs At Heliospheric Distances Beyond The Orbit Of Earth Are The Dominant Energetic Particle Population Observed In The Outer Heliosphere At These Times. Papers Included In This Volume Cover The Subject Of Cirs From Their Dissipation In The Outer Hemisphere, And Include Discussions Of Complexities Associated With Their Evolution With Distance From The Sun, Their Three-dimensional Structure, And The Myriad Effects That Cirs Have On Energetic Particles Throughout The Heliosphere. The Book Is Intended To Provide Scientists Active In Space Physics Research With An Up-to-date Status Report On Current Understanding Of Cirs And Their Effects In The Heliosphere, And Also To Serve The Advanced Graduate Student With Introductory Material On This Active Field Of Research. Edited By A. Balogh, J. T. Gosling, J. R. Jokipii, R. Kallenbach, H. Kunow. Front Matter....Pages i-xiv Introduction....Pages 1-3 Front Matter....Pages 5-5 Solar Origin and Interplanetary Evolution of Stream Interfaces....Pages 7-20 Formation and Evolution of Corotating Interaction Regions and Their Three Dimensional Structure....Pages 21-52 Voyager 2 Observations of Corotating Interaction Regions (CIRs) in the Outer Heliosphere....Pages 53-59 Development and Effects of Turbulence in Connection with CIRs....Pages 61-76 CIR Associated Energetic Particles in the Inner and Middle Heliosphere....Pages 77-90 Observation of Injection and Pre-Acceleration Processes in the Slow Solar Wind....Pages 91-104 Injection and Acceleration Processes in Corotating Interaction Regions: Theoretical Concepts....Pages 105-114 Mechansims for Latitudinal Transport of Energetic Particles in the Heliosphere....Pages 115-124 Modulation of Galactic Cosmic Rays at Solar Minimum....Pages 125-138 Front Matter....Pages 139-139 The Solar Origin of Corotating Interaction Regions and their Formation in the Inner Heliosphere....Pages 141-178 CIR Morphology, Turbulence, Discontinuities, and Energetic Particles....Pages 179-220 Corotating Interaction Regions at High Latitudes....Pages 221-268 Corotating Interaction Regions in the Outer Heliosphere....Pages 269-305 Modulation of Cosmic Rays and Anomalous Components by CIRs....Pages 307-326 Origin, Injection, and Acceleration of CIR Particles: Observations....Pages 327-367 Origin, Injection, and Acceleration of CIR Particles: Theory....Pages 369-399 Back Matter....Pages 401-411 Proceedings of an ISSI Workshop, 6-13 June 1998, Bern, Switzerland
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