Raspollini, Piera, Ade, Peter A. R. ![]() |
Abstract
A recovery procedure has been developed to correct instrument line-shape distortions observed in Fourier transform spectroscopy. The procedure can be described as a phase-error correction performed in the spectral domain to correct for path-difference-dependent phase errors observed in sharp spectral features. The technique has been applied successfully to high-resolution atmospheric emission spectra. The inherent broadening of the real features has been separated accurately from instrumental distortions. Using models for the path-difference-dependent error sources and data from two narrow window regions at 50 and 118 cm-1, we show that the distortion has a simple dependence on the spectral frequency.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Schools > Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | The Optical Society |
ISSN: | 0003-6935 |
Last Modified: | 27 Oct 2022 08:22 |
URI: | https://orca.cardiff.ac.uk/id/eprint/62097 |
Citation Data
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