Journal ArticleDOI
Absorption measurements of oxygen between 330 and 1140 nm
TLDR
The absorption spectrum of O2 and O2-O2 collision pairs were measured over the wavelength range from 330 to 1140 nm using pressures of O 2 from 1 to 55 atm at 298 K as mentioned in this paper.Abstract:
The absorption spectrum of O2 and O2-O2 collision pairs were measured over the wavelength range from 330 to 1140 nm using pressures of O2 from 1 to 55 atm at 298 K. Absorption cross sections, pressure dependences, band centers, and full widths at half maximum of the observed absorption bands centered at 343.4, 360.5, 380.2, 446.7, 477.3, 532.2, 577.2, 630.0, 688, 762, and 1065.2 nm are reported. The absorption bands centered at 360.5, 380.2, and 477.3 nm were also measured at 196 K and their temperature dependences were characterized.read more
Citations
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Journal ArticleDOI
The HITRAN 2008 molecular spectroscopic database
Laurence S. Rothman,Iouli E. Gordon,Yurii L. Babikov,A. Barbe,D. Chris Benner,Peter F. Bernath,Manfred Birk,Luca Bizzocchi,Vincent Boudon,Linda R. Brown,Alain Campargue,Kelly Chance,Edward A. Cohen,L. H. Coudert,V. M. Devi,Brian J. Drouin,André Fayt,Jean-Marie Flaud,Robert R. Gamache,Jeremy J. Harrison,Jean-Michel Hartmann,Christian Hill,Joseph T. Hodges,D. Jacquemart,Antoine Jolly,Julien Lamouroux,R. J. Le Roy,Gang Li,David A. Long,O.M. Lyulin,C.J. Mackie,Steven T. Massie,Semen Mikhailenko,Holger S. P. Müller,Olga V. Naumenko,Andrei Nikitin,Johannes Orphal,V.I. Perevalov,Agnes Perrin,E. R. Polovtseva,Charlotte Richard,Mary Ann H. Smith,Evgeniya Starikova,Keeyoon Sung,S.A. Tashkun,Jonathan Tennyson,Geoff Toon,Vl.G. Tyuterev,G. Wagner +48 more
TL;DR: The new HITRAN is greatly extended in terms of accuracy, spectral coverage, additional absorption phenomena, added line-shape formalisms, and validity, and molecules, isotopologues, and perturbing gases have been added that address the issues of atmospheres beyond the Earth.
Journal ArticleDOI
The hitran molecular spectroscopic database and hawks (hitran atmospheric workstation): 1996 edition
Laurence S. Rothman,Curtis P. Rinsland,A. Goldman,Steven T. Massie,David P. Edwards,Jean-Marie Flaud,Agnes Perrin,Claude Camy-Peyret,V. Dana,J.-Y. Mandin,J. Schroeder,A. Mccann,Robert R. Gamache,R. B. Wattson,Kouichi Yoshino,Kelly Chance,Kenneth W. Jucks,Linda R. Brown,V. Nemtchinov,Prasad Varanasi +19 more
TL;DR: The data and features that have been added or replaced since the previous edition of HITRAN are described, including instances of critical data that are forthcoming.
Journal ArticleDOI
Atmospheric radiative transfer modeling: a summary of the AER codes
Shepard A. Clough,Mark W. Shephard,Eli J. Mlawer,J. S. Delamere,Michael J. Iacono,Karen Cady-Pereira,Sid-Ahmed Boukabara,Patrick D. Brown +7 more
TL;DR: The line-by-line radiative transfer model (LBLRTM), the line file creation program (LNFL), RRTM_LW and RRTm_SW, Monochromatic Radiative Transfer Model (MonoRTM) as mentioned in this paper, MT_CKD Continuum; and the Kurucz Solar Source Function (SDF).
Journal ArticleDOI
The libRadtran software package for radiative transfer calculations (version 2.0.1)
Claudia Emde,Robert Buras-Schnell,Arve Kylling,Bernhard Mayer,Josef Gasteiger,Ulrich Hamann,Jonas Irgens Kylling,Jonas Irgens Kylling,Bettina Richter,Christian Pause,Timothy E. Dowling,Luca Bugliaro +11 more
TL;DR: The libRadtran as discussed by the authors software package is a widely used software package for radiative transfer calculations, which allows one to compute (polarized) radiances, irradiance, and actinic fluxes in the solar and thermal spectral regions.
Journal ArticleDOI
Multi axis differential optical absorption spectroscopy (MAX-DOAS)
TL;DR: In this paper, a Monte Carlo RTM is applied to calculate Airmass Factors (AMF) for the various viewing geometries of MAX-DOAS, which can be used to quantify the light path length within the absorber layers.
References
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Journal ArticleDOI
Visible spectroscopy at McMurdo Station, Antarctica: 2. Observations of OClO
TL;DR: The column abundance of OClO at McMurdo Station, Antarctica, was measured by visible absorption spectroscopy during austral spring in 1986 as discussed by the authors, which suggests that the halogen chemistry of Antarctic spring is profoundly different from such standard theoretical expectations and may play a role in the development of the springtime Antarctic ozone hole.
Journal ArticleDOI
Spectroscopic investigation of van der Waals molecules. I. The infrared and visible spectra of (O2)2
Charles A. Long,George E. Ewing +1 more
TL;DR: In this article, the infrared and visible spectra of gaseous oxygen have been examined at temperatures around 90°K using a long path absorption cell, and the visible absorption of (O2)2 corresponds to the 1 Δg (ν=0)+1 Δg(ν=1) ←3 Σg−(ν = 0) simultaneous transition.
Journal ArticleDOI
Visible and near-ultraviolet spectroscopy at McMurdo Station, Antarctica: 5. Observations of the diurnal variations of BrO and OClO
TL;DR: In this paper, the diurnal variations of OClO and BrO during austral spring, 1987, using long-path visible and near-ultraviolet absorption spectroscopy are presented and compared to simplified model calculations.
Journal ArticleDOI
Structure and energy transfer within isolated (O2)2 dimers via high resolution electronic spectroscopy
Julie Goodman,Louis E. Brus +1 more
TL;DR: In this paper, high-resolution 1Δg+1 Δg spectra have been observed in solid neon host at 4.2 K. The spectra are entirely consistent with D2h structure, and less likely with D 2d structure.
Journal ArticleDOI
Collision-induced absorption of O2 in the Herzberg continuum
Shardanand,A.D. Prasad Rao +1 more
TL;DR: Using a one meter normal incidence grating monochromator, the absorption cross sections of O2 and O4 were derived from total absorption measurements and compared with other available data as discussed by the authors.
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