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000751806 019__ $$a919341642$$a931592878$$a932333521
000751806 020__ $$a9783662483107$$q(electronic book)
000751806 020__ $$a3662483106$$q(electronic book)
000751806 020__ $$z9783662483091
000751806 020__ $$z3662483092
000751806 0247_ $$a10.1007/978-3-662-48310-7$$2doi
000751806 035__ $$aSP(OCoLC)ocn919123019
000751806 035__ $$aSP(OCoLC)919123019$$z(OCoLC)919341642$$z(OCoLC)931592878$$z(OCoLC)932333521
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000751806 049__ $$aISEA
000751806 050_4 $$aQC880.4.B65
000751806 08204 $$a551.5153$$223
000751806 1001_ $$aWang, Yi,$$eauthor.
000751806 24510 $$aMagnetic cloud boundary layers and magnetic reconnection$$h[electronic resource] /$$cYi Wang.
000751806 264_1 $$aHeidelberg :$$bSpringer,$$c[2016]
000751806 264_4 $$c©2016
000751806 300__ $$a1 online resource.
000751806 336__ $$atext$$btxt$$2rdacontent
000751806 337__ $$acomputer$$bc$$2rdamedia
000751806 338__ $$aonline resource$$bcr$$2rdacarrier
000751806 4901_ $$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$$x2190-5053
000751806 504__ $$aIncludes bibliographical references.
000751806 5050_ $$aSupervisor's Foreword; Acknowledgments; Contents; 1 Introduction; 1.1 Magnetic Reconnection; 1.1.1 Sweet-Parker Reconnection; 1.1.2 Hall Reconnection; 1.1.3 Petschek Reconnection; 1.1.4 Open Questions; 1.2 Particle Acceleration in Magnetic Reconnection; 1.2.1 Acceleration Region and Acceleration Process; 1.2.2 Acceleration Mechanism; 1.2.3 Open Questions; 1.3 Magnetic Cloud Boundary Layer; 1.3.1 The Identification of MC Boundary; 1.3.2 Properties of the BL; 1.3.3 Open Questions; 1.4 Magnetic Reconnection in the Solar Wind; 1.4.1 Structure of the Reconnection Exhaust
000751806 5058_ $$a1.4.2 Physical Properties of Magnetic Reconnections in the Solar Wind1.4.3 Open Questions; References; 2 Magnetic Reconnection and the Associated Energetic Particles in the Boundary Layer; 2.1 Introduction; 2.2 Analyzing Methods; 2.2.1 LMN Coordinate; 2.2.2 Walen Relation; 2.3 Magnetic Reconnection in the BL; 2.4 Energetic Particles Associated with Magnetic Reconnection; 2.5 Discussion and Conclusion; References; 3 The Acceleration of Energetic Particles in Magnetic Reconnection; 3.1 Introduction; 3.2 Background Description of Numerical Simulations
000751806 5058_ $$a3.2.1 Different Methods of Numerical Simulations3.2.2 GEM Magnetic Reconnection Challenge; 3.3 Simulation Results; 3.3.1 Interplanetary Magnetic Reconnection Driven by MC; 3.3.2 Acceleration of Energetic Electrons; 3.4 Discussion and Summary; References; 4 Proton and Electron Flux Variations in the Magnetic Cloud Boundary Layers; 4.1 Introduction; 4.2 The Velocity Distribution Function; 4.2.1 Definition of the Velocity Distribution Function; 4.2.2 The Moments of the Velocity Distribution Function; 4.2.3 Electron Velocity Distribution Function in Solar Wind; 4.3 Data Set Description
000751806 5058_ $$a4.3.1 Instruments and Data4.3.2 Event Selection; 4.4 Statistical Results; 4.5 Explanations for the Flux Variations at Different Energy Bands; 4.5.1 The Core Electrons; 4.5.2 The Suprathermal Electrons; 4.5.3 Energetic Electrons; 4.5.4 Protons; 4.6 Discussion and Summary; References; 5 The Criterion of Magnetic Reconnection in the Solar Wind; 5.1 Introduction; 5.2 Event Selection; 5.2.1 The Reconnection Exhaust; 5.2.2 The MC-Driven Shock; 5.3 Statistical Results; 5.4 Explanations for the Flux Variations in Different Events; 5.4.1 The Magnetic Cloud Boundary Layer and Reconnection Exhaust
000751806 5058_ $$a5.4.2 The MC-Driven Shock5.5 Discussion and Summary; References; 6 Summary and Outlook; References
000751806 506__ $$aAccess limited to authorized users.
000751806 520__ $$aThis thesis focuses on magnetic reconnection processes in the boundary layer of the interplanetary magnetic cloud. Magnetic reconnection is an important and frontier topic in the realm of physics. Various physical phenomena can be observed during the reconnection process but lots of them are not fully understood. This thesis provides the first observational evidence of energetic electrons associated with magnetic reconnection in the solar wind and discusses the particle acceleration problems. In addition, after analyzing the particle flux variations in Magnetic Cloud Boundary Layer, the thesis proposes a possible new criterion for the identification of magnetic reconnection in the solar wind. These tantalizing results could be particular clues to understand the dynamical problems in magnetic reconnection processes.
000751806 588__ $$aOnline resource; title from PDF title page (viewed August 26, 2015)
000751806 650_0 $$aBoundary layer (Meteorology)
000751806 650_0 $$aCosmic magnetic fields.
000751806 650_0 $$aSolar wind.
000751806 77608 $$iPrint version:$$z3662483092$$z9783662483091$$w(OCoLC)915120101
000751806 830_0 $$aSpringer Theses, Recognizing Outstanding Ph.D. Research.
000751806 852__ $$bebk
000751806 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-3-662-48310-7$$zOnline Access$$91397441.1
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000751806 980__ $$aBIB
000751806 982__ $$aEbook
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