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Brasunas J, Mamoutkine A, Gorius N. Simple parametric model for intensity calibration of Cassini composite infrared spectrometer data. Appl Opt. 2016;55(17):4699-705doi: 10.1364/AO.55.004699.
Brasunas, J., Mamoutkine, A., & Gorius, N. (2016). Simple parametric model for intensity calibration of Cassini composite infrared spectrometer data. Applied optics, 55(17), 4699-705. https://doi.org/10.1364/AO.55.004699
Brasunas, J, et al. "Simple parametric model for intensity calibration of Cassini composite infrared spectrometer data." Applied optics vol. 55,17 (2016): 4699-705. doi: https://doi.org/10.1364/AO.55.004699
Brasunas J, Mamoutkine A, Gorius N. Simple parametric model for intensity calibration of Cassini composite infrared spectrometer data. Appl Opt. 2016 Jun 10;55(17):4699-705. doi: 10.1364/AO.55.004699. PMID: 27409028.
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Appl Opt. 2016 Jun 10;55(17):4699-705. doi: 10.1364/AO.55.004699.

Simple parametric model for intensity calibration of Cassini composite infrared spectrometer data.

Applied optics

J Brasunas, A Mamoutkine, N Gorius

PMID: 27409028 DOI: 10.1364/AO.55.004699

Abstract

Accurate intensity calibration of a linear Fourier-transform spectrometer typically requires the unknown science target and the two calibration targets to be acquired under identical conditions. We present a simple model suitable for vector calibration that enables accurate calibration via adjustments of measured spectral amplitudes and phases when these three targets are recorded at different detector or optics temperatures. Our model makes calibration more accurate both by minimizing biases due to changing instrument temperatures that are always present at some level and by decreasing estimate variance through incorporating larger averages of science and calibration interferogram scans.

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