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The Wulf bands of oxygen

dc.contributor.authorBernath, P.
dc.contributor.authorCarleer, M.
dc.contributor.authorFally, S.
dc.contributor.authorJenouvrier, A.
dc.contributor.authorVandaele, A.C.
dc.contributor.authorHermans, C.
dc.contributor.authorMérienne, M.-F.
dc.contributor.authorColin, R.
dc.date1998
dc.date.accessioned2017-05-19T10:56:25Z
dc.date.available2017-05-19T10:56:25Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5394
dc.descriptionThe 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.
dc.languageeng
dc.titleThe Wulf bands of oxygen
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleChemical Physics Letters
dc.source.volume297
dc.source.issue3-4
dc.source.page293-299
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/S0009-2614(98)01149-X
dc.identifier.scopus2-s2.0-0013353558


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