Open AccessHigh‐temperature, high‐resolution photoabsorption cross sections of O 2 in the 108.5‐nm region
Author(s) -
Wu C. Y. Robert,
Hung T.,
Judge D. L.,
Matsui Takashi
Publication year - 2001
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2000ja000360
Subject(s) - airglow , absorption (acoustics) , ionosphere , absorption cross section , thermosphere , physics , resolution (logic) , cross section (physics) , materials science , atomic physics , analytical chemistry (journal) , optics , chemistry , astronomy , chromatography , artificial intelligence , computer science
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 this 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 located 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 The present room temperature cross‐section data of the N II 108.5‐nm sextuplets agree well with the unpublished data of J.A.R. Samson (private communication, 1990).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 the sharp features decrease as temperature increases. The N II 108.5‐nm multiplets are one of the prominent emissions in the Earth's airglow. The EUV‐UV day glow limb scans of the thermosphere and ionosphere have currently been gathered by satellite, e.g., ARGOS, at a tangent ray height of 200 km, above 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.