FIR and sub-mm direct detection spectrometers for spaceborne astronomy

Details FIR and sub-mm direct detection spectrometers for spaceborne astronomy FIR and sub-mm direct detection spectrometers for spaceborne astronomy

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990liaco..29..259w&link_type=abstract

In ESA, From Ground-Based to Space-Borne Sub-mm Astronomy p 259-263 (SEE N91-21986 13-89)

Astronomy and Astrophysics

Astronomy

Fabry-Perot Spectrometers, Far Infrared Radiation, Large Deployable Reflector, Satellite Instruments, Spaceborne Astronomy, Spaceborne Telescopes, Spectroscopic Telescopes, Submillimeter Waves, Astronomical Satellites, Fourier Transformation, Gratings (Spectra), Optical Filters

Scientific paper

Candidate spaceborne sub-mm instrumentation proposed for space projects with large passively cooled telescopes are reviewed. Grating instruments and Fourier transform spectroscopy (FTS) spectrometers are discussed. Particular attention is given to imaging Fabry-Perot spectrometers. The special needs of the Large Deployable Reflector (LDR) and for the Far InfraRed Space Telescope (FIRST) missions in this area are outlined. Possible Fabry-Perot spectrometer setups are diagrammed and outlined. The use of spherical and multiplex Fabry-Perot spectrometers is discussed.

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