Emission mechanism of /OI/ 557.7 nm radiation

Details Emission mechanism of /OI/ 557.7 nm radiation Emission mechanism of /OI/ 557.7 nm radiation

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jatp...42..299m&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 42, Mar. 1980, p. 299-302.

Physics

Emission Spectra, Forbidden Bands, Infrared Radiation, Molecular Spectra, Nightglow, Oxygen Spectra, Atmospheric Scattering, Hydroxyl Emission, Line Spectra, Oxygen Atoms

Scientific paper

An investigation is presented of the emission mechanism of /OI/ 557.7 nm line. It is based on a comparison of the correlation between the intensity changes of /OI/ 557.7 nm line and the O2(O-1) atmospheric band at 864.5 nm with the correlations between the intensity changes of the OH(6-2) and (8-3) bands which rise from the same emission mechanism. It was found that the correlation between the 557.7 nm line and the O2(O-1) is lower than that between the OH(6-2) and (8-3) bands, and that the correlation between the 557.7 nm line and the O2(0-1) shows a pronounced seasonal variation. It is concluded that the emission mechanism of the 557.7 nm line is the Chapman reaction (1931)

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