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    The Wulf bands of oxygen

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    Bernath(1998a).pdf (245.4Kb)
    Authors
    Bernath, P.
    Carleer, M.
    Fally, S.
    Jenouvrier, A.
    Vandaele, A.C.
    Hermans, C.
    Mérienne, M.-F.
    Colin, R.
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    Discipline
    Physical sciences
    Audience
    Scientific
    Date
    1998
    Metadata
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    Description
    The Wulf bands of oxygen in the 240-290 nm spectral region are caused by collision-induced absorption of the Herzberg III (A′3Δu-X3Σ- g) system. These bands had been previously attributed to the oxygen dimer, (O2)2. Under atmospheric conditions the Wulf bands are thus the long-wavelength extension of the Herzberg continuum. Absorption of solar radiation by the Wulf bands may be an additional source of NO in the stratosphere.
    Citation
    Bernath, P.; Carleer, M.; Fally, S.; Jenouvrier, A.; Vandaele, A.C.; Hermans, C.; Mérienne, M.-F.; Colin, R. (1998). The Wulf bands of oxygen. , Chemical Physics Letters, Vol. 297, Issue 3-4, 293-299, DOI: 10.1016/S0009-2614(98)01149-X.
    Identifiers
    uri: https://orfeo.belnet.be/handle/internal/5394
    doi: http://dx.doi.org/10.1016/S0009-2614(98)01149-X
    scopus: 2-s2.0-0013353558
    Type
    Article
    Peer-Review
    Yes
    Language
    eng
    Links
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