2000
DOI: 10.1006/jmsp.1999.8012
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Experimental Line Parameters of the Oxygen A Band at 760 nm

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Cited by 126 publications
(140 citation statements)
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“…Assuming that the broadening of the b 1 R þ g a 1 D g (0,0) band can be taken as the average of these two bands and that the experimental results can be extrapolated down to our 20 Torr experimental pressure, the rotational level average values reported by Cheah et al [7] yield a Lorentzian width of 0.0020 cm À1 . Similarly, Brown and Plymate [20] and Newman et al [6] derived rotational level specific broadening coefficients for the b 1 R þ g X 3 R À g ð0; 0Þ and a 1 D g X 3 R À g ð0; 0Þ bands, respectively. These coefficients yield a value of 0.0024 cm À1 for the Lorentzian full width of the Q(12) transition due to pressure broadening.…”
Section: Resultsmentioning
confidence: 98%
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“…Assuming that the broadening of the b 1 R þ g a 1 D g (0,0) band can be taken as the average of these two bands and that the experimental results can be extrapolated down to our 20 Torr experimental pressure, the rotational level average values reported by Cheah et al [7] yield a Lorentzian width of 0.0020 cm À1 . Similarly, Brown and Plymate [20] and Newman et al [6] derived rotational level specific broadening coefficients for the b 1 R þ g X 3 R À g ð0; 0Þ and a 1 D g X 3 R À g ð0; 0Þ bands, respectively. These coefficients yield a value of 0.0024 cm À1 for the Lorentzian full width of the Q(12) transition due to pressure broadening.…”
Section: Resultsmentioning
confidence: 98%
“…No studies have been performed that report the pressure-induced shifts and widths of these lines. However, some recent detailed studies involving the b 1 [7,20] and a 1 D g X 3 R À g IR atmospheric [6,7] bands have been reported. These studies were performed at pressures ranging from $100 to $760 Torr.…”
Section: Resultsmentioning
confidence: 99%
“…As can be seen in Fig. 1(a), the RR transitions for each isotopologue exhibit minimal 17 O-containing isotopologues with fit uncertainties. Each experimental Gaussian width was determined by a Levenberg-Marquardt least-squares fit using a single Voigt line shape with the pressure-broadening parameter constrained to the previously determined 16 O 2 value [12].…”
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confidence: 78%
“…Spectra were fit using Voigt line-shape profiles, which account for pressure (Lorentzian) and Doppler (Gaussian) broadening. The importance of using the Galatry [15] line profile for high-resolution measurements at higher pressures is well established [16,17]; however, due to the low pressures of this study, Dicke narrowing [18] is less than 1 MHz and was therefore neglected. During the fit, the transition position and intensity were floated while the pressure broadening coefficient was constrained to the 16 O 2 known values [12].…”
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confidence: 99%
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