Broadband, high-resolution investigation of advanced absorption line shapes at high temperature
Spectroscopic studies of planetary atmospheres and high-temperature processes (e.g., combustion) require absorption line-shape models that are accurate over extended temperature ranges. To date, advanced line shapes, like the speed-dependent Voigt and Rautian profiles, have not been tested above roo...
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Published in | Physical review. A Vol. 96; no. 2 |
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Main Authors | , , , , , , , |
Format | Journal Article |
Language | English |
Published |
United States
01.08.2017
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Online Access | Get more information |
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Summary: | Spectroscopic studies of planetary atmospheres and high-temperature processes (e.g., combustion) require absorption line-shape models that are accurate over extended temperature ranges. To date, advanced line shapes, like the speed-dependent Voigt and Rautian profiles, have not been tested above room temperature with broadband spectrometers. We investigate pure water vapor spectra from 296 to 1305 K acquired with a dual-frequency comb spectrometer spanning from 6800 to 7200 cm
at a point spacing of 0.0033 cm
and absolute frequency accuracy of
3.3 × 10
cm
. Using a multispectral fitting analysis, we show that only the speed-dependent Voigt accurately models this temperature range with a single power-law temperature-scaling exponent for the broadening coefficients. Only the data from the analysis using this profile fall within theoretical predictions, suggesting that this mechanism captures the dominant narrowing physics for these high-temperature conditions. |
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ISSN: | 2469-9926 |
DOI: | 10.1103/PhysRevA.96.022514 |