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This 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.
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Über die Autorin bzw. den Autor
Dr. Yi Wang
Education:
Ph.D. in Space Physics, University of Chinese Academy of Sciences, Beijing, China, June, 2012
B.S. in Space Physics, University of Science and Technology of China, Hefei, China, June, 2007
Professional Experience:
2012 July – present: Research Associate, National Space Science Center, Chinese Academy of Sciences, Beijing, China
Research Interests:
Magnetic reconnection and particle acceleration; waves and turbulence in the solar wind.
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This 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.
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Magnetic Cloud Boundary Layers and Magnetic Reconnection
Verlag:
Springer Berlin Heidelberg, 2015
ISBN 10: 3662483092
ISBN 13: 9783662483091
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Zustand: Sehr gut. Zustand: Sehr gut | Sprache: Englisch | Produktart: Bücher. Artikel-Nr. 26004841/12
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Magnetic Cloud Boundary Layers and Magnetic Reconnection
ISBN 10: 3662483092
ISBN 13: 9783662483091
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Hardcover
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Verkäuferbewertung 5 von 5 Sternen
Buch. Zustand: Neu. Neuware -This 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.Springer-Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 88 pp. Englisch. Artikel-Nr. 9783662483091
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Magnetic Cloud Boundary Layers and Magnetic Reconnection
Anbieter: AHA-BUCH GmbH, Einbeck, Deutschland
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Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - This 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. Artikel-Nr. 9783662483091
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