Transport calculations presented here are of photoelectron fluxes and energy spectra in the ionosphere for electrons along the magnetic field lines of the earth in an inhomogeneous anisotropically scattering atmosphere, which takes account of elastic, and inelastic collisions, and energy loss to ambient plasma. The transport fluxes at low altitudes are found to be lower than the local fluxes, while at high altitudes the transport fluxes are higher than the local fluxes. Results of our calculations are given and compared with the experimental data obtained from NASA Satellite Explorer C. The methodology used here is relatively new, interesting and powerful.