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Magnetic Cloud Boundary Layers and Magnetic Reconnection

Part of the Springer Theses Book Series

DOI: 10.1007/978-3-662-48310-7

ISBN: 978-3-662-48309-1

Publisher: Springer Berlin Heidelberg - Springer Journals

Aug 22, 2015

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Chapter 1Introduction

Wang, Yi

Pages: 1 –21

[Space physics studies various physical processes that exist in different regions including the middle and high layer atmosphere, ionosphere, magnetosphere, interplanetary space, the Sun, and the entire heliosphere.]
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Chapter 2Magnetic Reconnection and the Associated Energetic Particles in the Boundary Layer

Wang, Yi

Pages: 23 –33

[Previous studies have shown that BL is a turbulent layer formed by the interaction of the MC and the ambient solar wind (Wei et al. 2003a, b, c). Compared with those in the nearby upstream solar wind, the magnetic field in the BL is decreased and the plasma is compressed and heated.]
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Chapter 3The Acceleration of Energetic Particles in Magnetic Reconnection

Wang, Yi

Pages: 35 –44

[Magnetic reconnection acts as an efficient accelerator to generate energetic particles that could be found in the solar corona, solar wind, and magnetotail.]
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Chapter 4Proton and Electron Flux Variations in the Magnetic Cloud Boundary Layers

Wang, Yi

Pages: 45 –58

[Magnetic cloud boundary layer is a distinct region formed by the interaction of the magnetic cloud (MC) and the solar wind.]
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Chapter 5The Criterion of Magnetic Reconnection in the Solar Wind

Wang, Yi

Pages: 59 –70

[Ever since the “direct evidence” of magnetic reconnection in solar wind has been proposed by Gosling et al. (2005a), many reconnection exhausts are reported (Gosling et al. 2005a, b; Davis et al. 2006; Phan et al. 2006; Gosling et al. 2007a, b; Huttunen et al. 2007; Lavraud et al. 2009; Tian et...
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Chapter 6Summary and Outlook

Wang, Yi

Pages: 71 –72

[In this thesis, we carry out some researches related to magnetic reconnection and particle acceleration in the BL.]

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