The effects of drift and winds on the propagation of Galactic cosmic
  rays
  We study the effects of drift motions and the advection by a Galactic wind on
the propagation of cosmic rays in the Galaxy. We employ a simplified magnetic
field model, based on (and similar to) the Jansson-Farrar model for the
Galactic magnetic field. Diffusion is allowed to be anisotropic. The relevant
equations are solved numerically, using a set of stochastic differential
equations. Inclusion of drift and a Galactic wind significantly shortens the
residence time of cosmic rays, even for moderate wind speeds
