Design and mathematical modelling of the space-borne far-infrared Fourier transform spectrometer for REFIR experiment
Year: 1999
Authors: Palchetti L., Barbis A., Harries J.E., Lastrucci D.
Autors Affiliation: Ist. Ric. sulle Onde E., Via Panciatichi 64, I-50127 Florence, Italy; Alenia Difesa, Officine Galileo Unit, Space Division, Via Einstein 35, I-50013 Campi Bisenzio, Italy; Blackett Laboratory, Department of Physics, ICSTM, Prince Consort Road, London SW7 2BZ, United Kingdom
Abstract: A far infrared Fourier spectrometer named REFIR (Radiation explorer in the far infrared) has been designed for space-borne observations of the atmospheric radiance in the broad spectral range 100-1000 cm-1. The requirements are discussed and the adopted instrumental configuration is presented. The variability of the source and the narrow frequency bandwidth of the detectors as well as some novel features of the selected configuration require some dedicated analysis for the establishment of the instrument performances which are herewith described.
Journal/Review: INFRARED PHYSICS & TECHNOLOGY
Volume: 40 (5) Pages from: 367 to: 377
More Information: This work is part of the feasibility study of the REFIR instrument supported by D.G. XII of the European Commission under contract ENV4-CT96-0344. The authors wish to thank Prof. J. Leotin and Dr. D. Smirnov for providing information about detectors.KeyWords: Fourier transform infrared spectroscopy; Infrared detectors; Infrared spectrometers; Light polarization; Mathematical models, Spaceborne far infrared Fourier spectrometer, Fourier opticsDOI: 10.1016/S1350-4495(99)00026-2Citations: 20data from “WEB OF SCIENCE” (of Thomson Reuters) are update at: 2024-11-17References taken from IsiWeb of Knowledge: (subscribers only)Connecting to view paper tab on IsiWeb: Click hereConnecting to view citations from IsiWeb: Click here