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Magnetic Cloud Boundary Layers and Magnetic Reconnection

Wang Yi
Innbundet / 2015 / Engelsk

Produktdetaljer

ISBN
9783662483091
Publisert
2015-09-23
Utgiver
Vendor
Springer-Verlag Berlin and Heidelberg GmbH & Co. K
Høyde
235 mm
Bredde
155 mm
Aldersnivå
Research, P, 06
Språk
Product language
Engelsk
Format
Product format
Innbundet

Forfatter
Wang Yi

Biographical note

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.

Magnetic Cloud Boundary Layers and Magnetic Reconnection

Wang Yi
Innbundet / 2015 / Engelsk
Wang Yi
Innbundet / 2015 / Engelsk
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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.
Les mer
This thesis focuses on magnetic reconnection processes in the boundary layer of the interplanetary magnetic cloud. 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.
Les mer
Introduction.- Energetic electrons accelerated by magnetic reconnection in the solar wind.- The acceleration of energetic electrons in magnetic reconnection.- Proton and electron flux variation in the magnetic cloud boundary layers.- The criterion of magnetic reconnection in the solar wind.- Waves and turbulence associated with magnetic reconnection in the solar wind.- Summary and outlook.
Les mer
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.
Les mer
Provides the first observational evidence of energetic electrons associated with magnetic reconnection in the solar wind Proposes a combined acceleration model for the reconnection accelerated energetic electrons Suggests that flux variations, which are previously thought to have not enough relevance to magnetic reconnection, could be considered as an important signature of solar wind reconnection in the statistical point of view Includes supplementary material: sn.pub/extras
Les mer

Relaterte produkter

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.
Les mer
This thesis focuses on magnetic reconnection processes in the boundary layer of the interplanetary magnetic cloud. 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.
Les mer
Introduction.- Energetic electrons accelerated by magnetic reconnection in the solar wind.- The acceleration of energetic electrons in magnetic reconnection.- Proton and electron flux variation in the magnetic cloud boundary layers.- The criterion of magnetic reconnection in the solar wind.- Waves and turbulence associated with magnetic reconnection in the solar wind.- Summary and outlook.
Les mer
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.
Les mer
Provides the first observational evidence of energetic electrons associated with magnetic reconnection in the solar wind Proposes a combined acceleration model for the reconnection accelerated energetic electrons Suggests that flux variations, which are previously thought to have not enough relevance to magnetic reconnection, could be considered as an important signature of solar wind reconnection in the statistical point of view Includes supplementary material: sn.pub/extras
Les mer

Produktdetaljer

ISBN
9783662483091
Publisert
2015-09-23
Utgiver
Vendor
Springer-Verlag Berlin and Heidelberg GmbH & Co. K
Høyde
235 mm
Bredde
155 mm
Aldersnivå
Research, P, 06
Språk
Product language
Engelsk
Format
Product format
Innbundet

Forfatter
Wang Yi

Biographical note

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.

Relaterte produkter