  We present a simple model for electron transport in a possible layer of
exotic nuclear clusters (in the so called nuclear pasta layer) between the
crust and liquid core of a strongly magnetized neutron star. The electron
transport there can be strongly anisotropic and gyrotropic. The anisotropy is
produced by different electron effective collision frequencies along and across
local symmetry axis in domains of exotic ordered nuclear clusters and by
complicated effects of the magnetic field. We also calculate averaged kinetic
coefficients in case local domains are freely oriented. Possible applications
of the obtained results and open problems are outlined.
