(2014), Heater-induced ionization inferred from spectrometric airglow measurements, J. Geophys. Res. Space Physics, 119, 2038-2045, doi:10.1002 8, 557.7, 630.0, 777.4, and 844.6 nm were observed. On the basis of these emissions and using a methodology based on the method of Gilbert (1968, 1970), we estimate the suprathermal electron population and the subsequent equilibrium electron density profile, including contributions from electron impact ionization. We find that the airglow is consistent with heater-induced ionization in view of the spatial intermittency of the airglow.