作者: Henry H. Mantsch , Douglas J. Moffatt
DOI: 10.1007/978-94-011-1974-0_7
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摘要: Advances in FT-IR instrumentation have resulted the routine acquisition of infrared absorption spectra with signal-to-noise ratios excess 10,000. There are mathematical procedures that can make use this high ratio to calculate spectroscopic parameters prime importance spectroscopist: positions and intensities individual bands. In manuscript we describe, theory practice, two such techniques, Fourier self-deconvolution derivation, both which achieve band-narrowing at expense ratio.