High-Resolution Fourier-Transform Ultraviolet-Visible Spectrometer for the Measurement of Atmospheric Trace Species: Application to OH
Applied Optics, Vol. 40, Issue 12, pp. 2024-2030 (2001)
http://dx.doi.org/10.1364/AO.40.002024
Acrobat PDF (144 KB)
Abstract
A compact, high-resolution Fourier-transform spectrometer for atmospheric near-ultraviolet spectroscopy has been installed at the Jet Propulsion Laboratory’s Table Mountain Facility (34.4 °N, 117.7 °W, elevation 2290 m). This instrument is designed with an unapodized resolving power near 500,000 at 300 nm to provide high-resolution spectra from 290 to 675 nm for the quantification of column abundances of trace atmospheric species. The measurement technique used is spectral analysis of molecular absorptions of solar radiation. The instrument, accompanying systems designs, and results of the atmospheric hydroxyl column observations are described.
© 2001 Optical Society of America
[Optical Society of America ]
OCIS Codes
(010.1280) Atmospheric and oceanic optics : Atmospheric composition
(120.0280) Instrumentation, measurement, and metrology : Remote sensing and sensors
(300.6300) Spectroscopy : Spectroscopy, Fourier transforms
(300.6540) Spectroscopy : Spectroscopy, ultraviolet
Citation
Richard P. Cageao, Jean-Francois Blavier, James P. McGuire, Yibo Jiang, Vassilii Nemtchinov, Frank P. Mills, and Stanley P. Sander, "High-Resolution Fourier-Transform Ultraviolet-Visible Spectrometer for the Measurement of Atmospheric Trace Species: Application to OH," Appl. Opt. 40, 2024-2030 (2001)
http://www.opticsinfobase.org/ao/abstract.cfm?URI=ao-40-12-2024
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