Magnetic Cloud Boundary Layers and Magnetic Reconnection

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

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