  Magnetic reconnection is a fundamental process for releasing magnetic energy
in space physics and astrophysics. At present, the usual way to investigate the
reconnection process is through analytical studies or first-principles
numerical simulations. This paper is the first to understand the turbulent
magnetic reconnection process by exploring the nature of magnetic turbulence.
From the perspective of radio synchrotron polarization statistics, we study how
to recover the properties of the turbulent magnetic field by considering the
line of sight along different directions of the reconnection layer. We find
that polarization intensity statistics can reveal the spectral properties of
reconnection turbulence. This work opens up a new way of understanding
turbulent magnetic reconnection.
