Design of a far-infrared Fabry-Perot spectrometer for astronomy

Details Design of a far-infrared Fabry-Perot spectrometer for astronomy Design of a far-infrared Fabry-Perot spectrometer for astronomy

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993spie.1762..461j&link_type=abstract

Proc. SPIE Vol. 1762, p. 461-469, Infrared Technology XVIII, Bjorn F. Andresen; Freeman D. Shepherd; Eds.

Physics

Scientific paper

A cooled Fabry-Perot spectrometer working in the far-infrared the 350 and 450 micrometers wavelength atmospheric windows is presented. It is designed for low temperature operation (1.5 K), in vacuum. The reflecting surfaces (gold inductive grids) are deposited on monocrystalline quartz substrates. Three push-pull motors perform the scanning of the spectrometer.

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