1989
DOI: 10.1016/0301-0104(89)80152-1
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The collision-induced radiation of O2(a 1Δg)

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Cited by 22 publications
(17 citation statements)
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“…Under the same experimental conditions, no continuous emission was observed under the lines of the b -+ X bands (upper limit I 1% of the intensity of the discrete lines). Weak continua were observed under the lines of the 0-0 and 0-1 bands of the ulAK + X 3 2 ; system, confirming the results of a previous low-resolution study [28]. Measurements of the b -+ u band at low pressure and low resolution (10 cm-') showed that the form of the continuum is identical to that of the unresolved band.…”
Section: Results and Analysissupporting
confidence: 86%
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“…Under the same experimental conditions, no continuous emission was observed under the lines of the b -+ X bands (upper limit I 1% of the intensity of the discrete lines). Weak continua were observed under the lines of the 0-0 and 0-1 bands of the ulAK + X 3 2 ; system, confirming the results of a previous low-resolution study [28]. Measurements of the b -+ u band at low pressure and low resolution (10 cm-') showed that the form of the continuum is identical to that of the unresolved band.…”
Section: Results and Analysissupporting
confidence: 86%
“…According to this hypothesis, the relative efficiencies of different collision partners in inducing the b --f a and a + X transitions of 0 2 should go in parallel. Hitherto, accurate rate constants for collision-induced emission of the a + X transition have been measured only for Oz and NO as collision partners [28,29]. However, preliminary measurements have shown that the rare gases Ar and Kr as well as NZ, SF,, SOz, and PC13 are much less efficient than is Oz in inducing a + X emission (kc 5 cm3 s-l [29])*.…”
Section: Discussionmentioning
confidence: 97%
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“…Several other less direct measurements of the rate coefficient agree with the recommendation, including Clark and Wayne [270], Findlay et al [453], and McLaren et al [894]. Wildt et al [1456] report observations of weak emissions in the near IR due to collision-induced radiation. Wildt et al [1457] give rate coefficients for this process.…”
Section: Notes Tomentioning
confidence: 49%