1967
DOI: 10.1016/0020-0891(67)90026-7
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Auxiliary computation for Fourier spectrometry

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Cited by 190 publications
(72 citation statements)
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“…The Bruker IFS 120HR Fourier transform spectrometer (FTS) was configured with a 150 W quartz tungsten halogen source, a calcium fluoride beam-splitter, and a liquid nitrogen-cooled indium antimonide (InSb) detector. Mertz phase correction [4] was applied to the measured interferograms. Optical filters were used to limit the optical bandwidth to the spectral range of the measurement.…”
Section: Methodsmentioning
confidence: 99%
“…The Bruker IFS 120HR Fourier transform spectrometer (FTS) was configured with a 150 W quartz tungsten halogen source, a calcium fluoride beam-splitter, and a liquid nitrogen-cooled indium antimonide (InSb) detector. Mertz phase correction [4] was applied to the measured interferograms. Optical filters were used to limit the optical bandwidth to the spectral range of the measurement.…”
Section: Methodsmentioning
confidence: 99%
“…Our interferogram processing currently includes a solar intensity variation correction (described below), a phase correction described by Forman et al [45], but with a convolution in the spectral domain as described by Mertz [46,47], and a fast Fourier transform based on the work of Bergland [48]. The InGaAs and Si detectors are sufficiently linear that no nonlinearity correction is required.…”
Section: (B) Interferogram Processingmentioning
confidence: 99%
“…After each day of measurements, the interferograms are assessed visually by the operator to check for data quality to remove any periods of total cloud contamination. The raw interferograms are then processed by the I2S (interferogramto-spectrum) software package, which corrects for solar intensity fluctuations (Keppel-Aleks et al, 2007), applies a phase correction (Mertz, 1967) and a laser sampling error (LSE) correction (Sect. 4.1 below), and then computes the spectra using a fast Fourier transform (Bergland, 1969).…”
Section: Data Processingmentioning
confidence: 99%