1987
DOI: 10.1029/ja092ia07p07753
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Comment on “The O2 atmospheric dayglow in the thermosphere” by M. R. Torr, B. Y. Welsh, and D. G. Torr

Abstract: It is known that v'-2-5 of O2(b ) are generated in aurorae, and possible mechanisms for this process are discussed in a recent paper [Slanger, 1986], drawing from earlier suggestions by Vallance Jones [1974, 1975] and $wider [1974]. However, the study of Torr et al. [1986] is the first to suggest that there are significant emissions from these levels in the dayglow.Unfortunately, no spectral simulation was performed, and

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Cited by 5 publications
(6 citation statements)
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“…Reagent gases are introduced into the reaction cell through temperature-controlled feed lines, as shown in Figure 1. N(2D,2P) are produced (together with N(4S) and excited metastable states of N2) by passing a flowing N2/Ar mixture at approximately 1 Torr through four parallel microwave discharges (2450 MHz, 50 W) prior to expanding into a low-pressure (approximately 3 mTorr), cryogenically pumped interaction volume. A counterflow gas (02 or Ar) enters the volume from the opposite side to combine with the discharge-excited gas in a stagnation region along the axis of the cell, which coincides with the axis of the cylindrical field of view of the detection system.…”
Section: Experimental Measurementsmentioning
confidence: 99%
“…Reagent gases are introduced into the reaction cell through temperature-controlled feed lines, as shown in Figure 1. N(2D,2P) are produced (together with N(4S) and excited metastable states of N2) by passing a flowing N2/Ar mixture at approximately 1 Torr through four parallel microwave discharges (2450 MHz, 50 W) prior to expanding into a low-pressure (approximately 3 mTorr), cryogenically pumped interaction volume. A counterflow gas (02 or Ar) enters the volume from the opposite side to combine with the discharge-excited gas in a stagnation region along the axis of the cell, which coincides with the axis of the cylindrical field of view of the detection system.…”
Section: Experimental Measurementsmentioning
confidence: 99%
“…Although, simultaneously with the O 2 (a 1 ∆ g , v = 0) and O 2 (b 1 Σ + g , v = 0) levels, the electronic-vibrational levels of oxygen molecules with v ≥ 1 are populated. Emission transitions from the O 2 (a 1 ∆ g , v ≥ 0) and O 2 (b 1 Σ + g , v ≥ 0) are observed in the atmospheric glow and clearly correlate with each other [12,[22][23][24]. Note that emission bands of an oxygen molecule with much higher levels of vibrational excitation O 2 (b 1 Σ + g , v = 0-15) are also observed in the atmospheric glow [25].…”
mentioning
confidence: 72%
“…O2(b 1 Σg + , v = 2) + О3 → O2(a 1 Δg, v = 2) + O3(203) + 2.0 cm −1 (12) Of particular interest are the collisional reactions of electronically-vibrationally excited oxygen molecules with atomic oxygen. To date, the products of these reactions are not known, however, their rate coefficients have a rather large scatter of values (see Table 2).…”
Section: Energy Transfer In Collisional Reactionsmentioning
confidence: 99%
“…Torr et al [19] suggested the production mechanism of 0 D 2-4 to be energy transfer between N( 2 D) and O 2 . Slanger et al [22] later argued that this proposed mechanism needs to be reinvestigated by examining the observed spectra to include all other possible emission features present in the observed spectra. In the analysis of auroral O 2 (1-1) and (0-1) emission intensities and temperatures, Sivjee et al [23] examined the auroral O 2 ( 1 †, 0 ) sources in the O( 1 D) + O 2 reaction and interpreted them using the production yields obtained in the laboratory by Lee and Slanger [24].…”
Section: The O 2 Atmospheric Band Emissionmentioning
confidence: 95%