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Use Of A Fourier Transform Spectrometer On A Balloon-Borne Telescope And At The Multiple Mirror Telescope (MMT)
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Use Of A Fourier Transform Spectrometer On A Balloon-Borne Telescope And At The Multiple Mirror Telescope (MMT)
Use Of A Fourier Transform Spectrometer On A Balloon-Borne Telescope And At The Multiple Mirror Telescope (MMT)
WT
W. A. Traub
W. A. Traub
K. V. Chance
K. V. Chance
JB
J. C. Brasunas
J. C. Brasunas
JV
J. M. Vrtilek
J. M. Vrtilek
NC
N. P. Carleton
N. P. Carleton
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16 November 1982
conference paper
Published by
SPIE-Intl Soc Optical Eng
Vol. 331
,
208-218
https://doi.org/10.1117/12.933457
Abstract
We describe the design and use of an infrared Fourier transform spectrometer which has been used for observations of laboratory, stratospheric, and astronomical spectra. The spectrometer has a spectral resolution of 0.032 cm and has operated in the mid-infrared (12 to 13 microns) as well as the far-infrared (40 to 140 microns), using both bolometer and photoconductor cryogenic detectors. The spectrometer is optically sized to accept an f/9 beam from the multi-mirror telescope (MMT). The optical and electronic design are discussed, including remote operation of the spectrometer on a balloon-borne 102 cm telescope. The performance of the laser-controlled, screw-driven moving cat's-eye mirror is discussed. Segments of typical far-infrared balloon flight spectra, lab spectra, and mid-infrared MMT spectra are presented. Data reduction, interferogram processing, artifact removal, wavelength calibration, and intensity calibration methods are discussed. Future use of the spectrometer is outlined.© (1982) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Keywords
INFRARED ASTRONOMY
SPECTROMETERS
FOURIER TRANSFORMATION
RADIATION DETECTORS
SIGNAL PROCESSING
SPECTRAL RESOLUTION
PHOTORESISTORS
FAR INFRARED
FOURIER TRANSFORMS
BOLOMETERS
DATA PROCESSING
CALIBRATION
LASERS
SENSORS
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Cited by 6 articles