  The magnetic topology and field line random walk properties of a
nanoflare-heated and magnetically confined corona are investigated in the
reduced magnetohydrodynamic regime. Field lines originating from current sheets
form coherent structures, called Current Sheet Connected (CSC) regions,
extended around them. CSC field line random walk is strongly anisotropic, with
preferential diffusion along the current sheets' in-plane length. CSC field
line random walk properties remain similar to those of the entire ensemble but
exhibit enhanced mean square displacements and separations due to the stronger
magnetic field intensities in CSC regions. The implications for particle
acceleration and heat transport in the solar corona and wind, and for solar
moss formation are discussed.
