Design and mathematical modelling of the space-borne far-infrared Fourier transform spectrometer for REFIR experiment (Articolo in rivista)

Type
Label
  • Design and mathematical modelling of the space-borne far-infrared Fourier transform spectrometer for REFIR experiment (Articolo in rivista) (literal)
Anno
  • 1999-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1016/S1350-4495(99)00026-2 (literal)
Alternative label
  • Palchetti, L and Barbis, A and Harries, JE and Lastrucci, D (1999)
    Design and mathematical modelling of the space-borne far-infrared Fourier transform spectrometer for REFIR experiment
    in Infrared physics & technology; Elsevier Science Publishers B.V., Amsterdam (Paesi Bassi)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Palchetti, L and Barbis, A and Harries, JE and Lastrucci, D (literal)
Pagina inizio
  • 367 (literal)
Pagina fine
  • 377 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 40 (literal)
Rivista
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroFascicolo
  • 5 (literal)
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • Palchetti, L (Reprint Author), Ist Ric Onde Elettromagnet Nello Carrara, Via Panciatichi 64, I-50127 Florence, Italy. Ist Ric Onde Elettromagnet Nello Carrara, I-50127 Florence, Italy. Alenia Difesa, Officine Galileo Unit, Space Div, I-50013 Campi Bisenzio, Italy. Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Dept Phys, London SW7 2BZ, England. (literal)
Titolo
  • Design and mathematical modelling of the space-borne far-infrared Fourier transform spectrometer for REFIR experiment (literal)
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. (C) 1999 Elsevier Science B.V. All rights reserved. (literal)
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