The UV spectra over the southern hemisphere nightside auroral oval have been obtained from an AFGL spectral/photometric experiment on board the low-altitude polar-orbiting S3--4 satellite. A detailed analysis of nightside auroral spectra from seven orbits between mid-May and June 1978 was performed to estimate the average energy and total energy flux of incident electrons. This study was based on observations of the N2 LBH (3--10) (1928 ¿) band and the N2 VK (0--5) (2604 ¿) band emission intensities and the application of model calculations by Strickland et al. [1983> and Daniell and Strickland [1986>. Comparison of the estimated quantities with the statistical satellite measurement of incident particles by Hardy et al. [1985> indicates that the LBH (3--10) band emission intensity can be used to estimate the total energy flux of incident electrons, similar to the N2+ 1N (0--0) (3914 ¿) band emission intensity in the visible region. In addition, the ratio of the BLH (3--10) to the VK (0--5) band emission intensities indicates the average energy of incident auroral electrons in much the same way that the N2+ IN (0--0) and O I (6300 ¿) emission ratio does in the visible region. This study shows the use of different constituent emissions, model calculations, and synthetic spectra to infer the inherent possibilities in these types of studies. ¿ American Geophysical Union 1988