Abstract
The increase of the emission intensity of the chemiluminescent reaction due to a third body M was first shown in 1967 in the pressure region of 3 to 20 mTorr (Becker et al., 1967, 1968a). Although these findings were confirmed independently by two other groups (Jonathan and Petty, 1968; McKenzie and Thrush, 1968), experimental limitations did not permit interpreting these results as definitive evidence against a two-body mechanism for the airglow reaction in the pressure region of 1 to 100 mTorr (Reeves et al., 1964).
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© 1971 D. Reidel Publishing Company, Dordrecht-Holland
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Becker, K.H., Groth, W., Thran, D. (1971). The Airglow Reaction NO+O+(M)→NO *2 at Low Pressures. In: Fiocco, G. (eds) Mesospheric Models and Related Experiments. Astrophysics and Space Science Library, vol 25. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3114-1_21
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DOI: https://doi.org/10.1007/978-94-010-3114-1_21
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