Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published June 3, 2004 | Supplemental Material
Journal Article Open

Temperature and Pressure Dependence of High-Resolution Air-Broadened Absorption Cross Sections of NO_2(415−525 nm)

Abstract

Cross sections of air-broadened NO_2 in the 415−525 nm region are reported. These are retrieved from 21 absorption spectra recorded at 0.060 cm^(-1) resolution with the McMath−Pierce Fourier Transform Spectrometer located on Kitt Peak in Arizona. The measurements are obtained for pressures (1−760 Torr) and temperatures (220−298 K) that are representative of typical tropospheric and stratospheric conditions. Two sigma uncertainty (95% confidence interval ≈ 2σ_(mean)) for the absolute absorption cross sections is below ±7% over the reported wavelength range. The average integrated intensity of all our data is 〈σ〉_(400-500 nm) = 4.53 × 10^(-17) cm^2 nm, which is within 0.2% of the averaged value from the recent literature. The wavelength (referred to vacuum) accuracy is 0.011 cm^(-1) (2.8 × 10^(-4) nm at 500 nm) and precision is 0.0022 cm^(-1) throughout the investigated wavelength range. In agreement with previous observations, high-resolution features in the NO_2 absorption spectrum display a strong pressure dependence with an effective pressure broadening parameter of 0.116 ± 0.003 cm^(-1)/atm (the rate of increase of Lorentzian half width at half-maximum with pressure). Temperature has a relatively minor effect on the shapes of individual high-resolution features, but it exerts a complex dependence on the relative line intensities. Absorption cross sections reported here represent the highest resolution data available over a substantial (>100 nm) wavelength range for quantitative analysis of NO_2 atmospheric column absorption spectra.

Additional Information

© 2004 American Chemical Society. Received 5 February 2004. Published online 8 May 2004. Published in print 1 June 2004. This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This work was supported by the NASA EOS/Aura Validation, Upper Atmosphere Research and Tropospheric Chemistry Programs. S.A.N. thanks the Camille and Henry Dreyfus Foundation for the postdoctoral scholarship. The authors thank M. Dulick for experimental assistance and G. Mount and J. Harder for helpful discussions.

Attached Files

Supplemental Material - jp049461nsi20040505_045414.pdf

Supplemental Material - jp049461nsi20040505_045615.zip

Supplemental Material - jp049461nsi20040505_050537.zip

Supplemental Material - jp049461nsi20040505_050625.zip

Supplemental Material - jp049461nsi20040505_050737.zip

Supplemental Material - jp049461nsi20040505_050857.zip

Supplemental Material - jp049461nsi20040505_050941.zip

Supplemental Material - jp049461nsi20040505_073127.zip

Supplemental Material - jp049461nsi20040505_073153.zip

Supplemental Material - jp049461nsi20040505_073211.zip

Supplemental Material - jp049461nsi20040505_073229.zip

Supplemental Material - jp049461nsi20040505_073245.zip

Supplemental Material - jp049461nsi20040505_073310.zip

Supplemental Material - jp049461nsi20040505_073331.zip

Supplemental Material - jp049461nsi20040505_073348.zip

Supplemental Material - jp049461nsi20040505_073408.zip

Supplemental Material - jp049461nsi20040505_073424.zip

Supplemental Material - jp049461nsi20040505_073500.zip

Supplemental Material - jp049461nsi20040505_073526.zip

Supplemental Material - jp049461nsi20040505_073648.zip

Supplemental Material - jp049461nsi20040505_073734.zip

Supplemental Material - jp049461nsi20040505_073810.zip

Supplemental Material - jp049461nsi20040505_073823.zip

Supplemental Material - jp049461nsi20040505_073838.zip

Supplemental Material - jp049461nsi20040505_073856.zip

Supplemental Material - jp049461nsi20040505_073919.zip

Files

jp049461nsi20040505_073526.zip
Files (12.5 MB)
Name Size Download all
md5:35a91ebaefabbd95571c277f649f5752
476.3 kB Preview Download
md5:5aa05d05bbb6b1ebd3f4f878d14fca19
490.4 kB Preview Download
md5:733656286ecdcc54b74710b0c4a6ddc1
475.3 kB Preview Download
md5:cd23dae7b0510b367eb40a948e061e3c
838.9 kB Preview Download
md5:040642560fca57926646baae88f219a6
465.2 kB Preview Download
md5:2c35b3387c1029d86551134c06d5e808
469.7 kB Preview Download
md5:df4301296b857da8aa4ac10b1c5a2001
493.5 kB Preview Download
md5:58b2704b1dd312b47d74d6fd08f9681a
491.1 kB Preview Download
md5:d979a2afc8bb24536e446141071e511f
476.7 kB Preview Download
md5:6a4c9dc11d48ffe8eee9399bad54ef54
472.4 kB Preview Download
md5:7838fba497b0753fd4effbb90482a442
473.7 kB Preview Download
md5:f3d48dd6bb330edb3a90d64e1da05e31
438.1 kB Preview Download
md5:3aae09a0b4edd7c0ed04680463dbae39
484.3 kB Preview Download
md5:9ae815187a733a2a30bcd59eab2ca258
151.5 kB Preview Download
md5:94ff2507119307361a13af8198fc32fe
431.7 kB Preview Download
md5:290ee9241c4392379b092059af45ad6d
450.8 kB Preview Download
md5:fd288c0b2b94ceb02270f423dcf94345
480.3 kB Preview Download
md5:73bdc7e60ad2f39abcf61e8c59e61ce3
439.1 kB Preview Download
md5:85b36e5db5afeaf5d4aabb32fcdc74bc
503.9 kB Preview Download
md5:d9f34951ec906a6152fb0a1bbf73046b
487.8 kB Preview Download
md5:ab95d013b5150702683f997d30ba31d9
453.5 kB Preview Download
md5:e45b628add31c892f0927525c50a463c
489.8 kB Preview Download
md5:2c17e2f7850938afbdc126957364a00f
497.9 kB Preview Download
md5:5e47b2ae2736dbaa4c337d7d1c90f19f
507.1 kB Preview Download
md5:65b2fc6eef91038ac285e9ed2d43571f
513.9 kB Preview Download
md5:524edf756c48be483e4f2a7cf0ad698a
497.5 kB Preview Download

Additional details

Created:
August 19, 2023
Modified:
October 25, 2023