A high-resolution, low-energy electron spectrometer can be deployed on
rockets or satellites to measure absolute spacecraft floating potenti
al relative to true (Earth) ground with an accuracy of +/-0.2 V. Featu
res due to the photoionization of nitrogen and atomic oxygen by an ext
remely sharp solar extreme ultraviolet line (304 Angstrom, He II) appe
ar in the electron spectra collected by the instrument. At altitudes w
here the photoelectron production is local (below 250 km), the peaks t
hat appear in tile spectrum are created by electrons of a known kineti
c energy: the energy of the ionizing photon minus the energy needed to
ionize either atomic oxygen or molecular nitrogen, The spacecraft pot
ential is determined from the apparent shift in the energy of the phot
oelectron spectral peaks. The instrument is best suited for use in the
daytime atmosphere at altitudes between 150 and 250 km. The spectrome
ter is based on an earlier design, that of the photoelectron spectrome
ter of the Atmosphere Explorer satellites. Enhancements of the earlier
design, including a threefold greater throughput and a specialized sc
an mode, greatly improve the determination of spacecraft potential. Ti
le placement of the instrument on the spacecraft is critical to the su
ccess of the measurements.