Full Description
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.
Contents
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.
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