All the available nightside electron data obtained during circular orb
its at Mars from the Phobos-2 HARP instrument have been examined in de
tail and are summarized in this paper. An electron flux component with
energies exceeding that of the unperturbed solar wind was observed in
side the magnetosheath, indicating the presence of acceleration mechan
ism(s). The character of the electron fluxes measured in the magnetota
il cannot be classified in any simple manner, however, there is a corr
elation between the electron fluxes measured well inside this region a
nd the unperturbed solar wind ram pressure.