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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.

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The HITRAN 2008 molecular spectroscopic database

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

Atmospheric radiative transfer modeling: a summary of the AER codes

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)

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.
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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.
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Spectroscopic investigation of van der Waals molecules. I. The infrared and visible spectra of (O2)2

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.
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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.
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Structure and energy transfer within isolated (O2)2 dimers via high resolution electronic spectroscopy

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

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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