The high-resolution absorption cross-section measurements of O-2 in the 108
.0-to 108.7-nm spectral region have been carried out with a resolution of 0
.0008 nm and at temperatures of 295 and 535 K. The absorption features in t
his spectral region exhibit primarily a blue-shaded broad band with a band
head peaked at 108.52 nm. The center of gravity of the diffuse band is loca
ted at 108.452 nm. The present room temperature cross-section data of the N
-II 108.5-nm sextuplets agree well with the unpublished data of J.A.R. Sams
on (private communication, 1990). As the temperature increases from 295 to
535 K, we observe a decrease in cross-section values by as much as 30% over
the contour of the diffuse band. Similarly, the cross-section values of th
e sharp features decrease as temperature increases. The N-II 108.5-nm multi
plets are one of the prominent emissions in the Earth's airglow. The EUV-UV
dayglow limb scans of the thermosphere and ionosphere have currently been
gathered by satellite, e.g., ARGOS, at a tangent ray height of 200 km, abov
e where the ambient absorption due to O-2 and N-2 is expected. The present
temperature-dependent cross sections of O-2 provide the important database
required for modeling the dayglow observations.