  Drift effects play a significant role in the transport of charged particles
in the heliosphere. A turbulent magnetic field is also known to reduce the
effects of particle drifts. The exact nature of this reduction, however, is not
clear. This study aims to provide some insight into this reduction, and
proposes a relatively simple, tractable means of modelling it that provides
results in reasonable agreement with numerical simulations of the drift
coefficient in a turbulent magnetic field.
