2019
DOI: 10.1364/oe.27.037920
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Baseline-free quantitative absorption spectroscopy based on cepstral analysis

Abstract: The accuracy of quantitative absorption spectroscopy depends on correctly distinguishing molecular absorption signatures in a measured transmission spectrum from the varying intensity or 'baseline' of the light source. Baseline correction becomes particularly difficult when the measurement involves complex, broadly absorbing molecules or non-ideal transmission effects such as etalons. We demonstrate a technique that eliminates the need to account for the laser intensity in absorption spectroscopy by converting… Show more

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Cited by 64 publications
(40 citation statements)
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“…While the average intensity fluctuates significantly due to beam steering, the spectral distribution of the background intensity (I 0 ) remains quite stable (see Figure 2a). Broadband fluctuations, probably caused by beam steering and interference fringes, as shown in the overlapping spectra, can be automatically compensated for during data evaluation, for example, by differentiation [27], Bayesian inference and fringe modeling [34], or a Fast Fourier Transformation [35]. For most of the measurements, a larger fraction of overexposed frames is observed, as visualized in the temporal course of the average camera intensity (Figure 2b).…”
Section: Methodsmentioning
confidence: 99%
“…While the average intensity fluctuates significantly due to beam steering, the spectral distribution of the background intensity (I 0 ) remains quite stable (see Figure 2a). Broadband fluctuations, probably caused by beam steering and interference fringes, as shown in the overlapping spectra, can be automatically compensated for during data evaluation, for example, by differentiation [27], Bayesian inference and fringe modeling [34], or a Fast Fourier Transformation [35]. For most of the measurements, a larger fraction of overexposed frames is observed, as visualized in the temporal course of the average camera intensity (Figure 2b).…”
Section: Methodsmentioning
confidence: 99%
“…In E -binning, one species is split into several distinct absorption models (of all the absorption features with similar E ), and the fit coefficients for each signature are the normalized linestrengths at each E bin. Because E -binning works the same as a multispecies fit, we can use modified free induction decay (m-FID) fitting [30] to separate the laser intensity baseline from most of the absorption signal, and determine the normalized linestrengths by linear regression. We can then use the inversion method in the companion paper to solve for a temperature distribution that fits a convex curve to the normalized linestrengths.…”
Section: Fitting Normalized Linestrengthsmentioning
confidence: 99%
“…Laser-absorption spectroscopy (LAS) is widely used to provide non-invasive measurements of temperature, chemical species, pressure, and velocity. The demand for LAS measurements in high pressure and highly transient combustion and propulsion environments (e.g., detonation engines, rocket motors) continues to propel innovations in LAS diagnostics [1,2,3,4,5] and data-processing techniques [6,7,8]. Several of these innovations have focused on increasing the usable spectral bandwidth of LAS diagnostics while maintaining or improving temporal resolution.…”
Section: Introductionmentioning
confidence: 99%