High-temperature, high-resolution photoabsorption cross sections of O-2 inthe 108.5-nm region

Citation
Cyr. Wu et al., High-temperature, high-resolution photoabsorption cross sections of O-2 inthe 108.5-nm region, J GEO R-S P, 106(A4), 2001, pp. 5599-5603
Citations number
34
Categorie Soggetti
Space Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN journal
21699380 → ACNP
Volume
106
Issue
A4
Year of publication
2001
Pages
5599 - 5603
Database
ISI
SICI code
0148-0227(20010401)106:A4<5599:HHPCSO>2.0.ZU;2-M
Abstract
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 The present room temperature cross-section data of the N -II 108.5-nm sextuplets agree well with the unpublished data of J.A.R. Sams on (private communication, 1990).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.