The Wulf bands of oxygen

P  Bernath; M  Carleer; S  Fally; A  Jenouvrier; A C  Vandaele; C  Hermans; M F  Merienne; R  Colin

The Wulf bands of oxygen

P Bernath, M Carleer, S Fally, A Jenouvrier, A C Vandaele, C Hermans, M F Merienne, R Colin

Chemistry

Research output: Contribution to journal › Article › peer-review

Abstract

The Wulf bands of oxygen in the 240-290 nm spectral region are caused by collision-induced absorption of the Herzberg III (A'(3)Delta(u)-X(3)Sigma(g)(-)) system. These bands had been previously attributed to the oxygen dimer, (O-2)(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. (C) 1998 Elsevier Science B.V. All rights reserved.

Original language	English
Pages (from-to)	293-299
Number of pages	7
Journal	Chemical Physics Letters
Volume	297
Issue number	3-4
Publication status	Published - 27 Nov 1998

Keywords

GAS-PHASE

Cite this

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title = "The Wulf bands of oxygen",

abstract = "The Wulf bands of oxygen in the 240-290 nm spectral region are caused by collision-induced absorption of the Herzberg III (A'(3)Delta(u)-X(3)Sigma(g)(-)) system. These bands had been previously attributed to the oxygen dimer, (O-2)(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. (C) 1998 Elsevier Science B.V. All rights reserved.",

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author = "P Bernath and M Carleer and S Fally and A Jenouvrier and Vandaele, {A C} and C Hermans and Merienne, {M F} and R Colin",

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language = "English",

volume = "297",

pages = "293--299",

journal = "Chemical Physics Letters",

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TY - JOUR

T1 - The Wulf bands of oxygen

AU - Bernath, P

AU - Carleer, M

AU - Fally, S

AU - Jenouvrier, A

AU - Vandaele, A C

AU - Hermans, C

AU - Merienne, M F

AU - Colin, R

PY - 1998/11/27

Y1 - 1998/11/27

N2 - The Wulf bands of oxygen in the 240-290 nm spectral region are caused by collision-induced absorption of the Herzberg III (A'(3)Delta(u)-X(3)Sigma(g)(-)) system. These bands had been previously attributed to the oxygen dimer, (O-2)(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. (C) 1998 Elsevier Science B.V. All rights reserved.

AB - The Wulf bands of oxygen in the 240-290 nm spectral region are caused by collision-induced absorption of the Herzberg III (A'(3)Delta(u)-X(3)Sigma(g)(-)) system. These bands had been previously attributed to the oxygen dimer, (O-2)(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. (C) 1998 Elsevier Science B.V. All rights reserved.

KW - GAS-PHASE

M3 - Article

SN - 0009-2614

VL - 297

SP - 293

EP - 299

JO - Chemical Physics Letters

JF - Chemical Physics Letters

IS - 3-4

ER -