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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