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Proceedings Paper

Miniaturized, 9--12 um heterodyne spectrometer with space qualifiable design features
Author(s): David Alan Glenar; M. J. Mumma; Theodore Kostiuk; H. Huffman; John J. Degnan; Hemant H. Dave; Urs E. Hochuli; Paul R. Haldemann
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Paper Abstract

A demonstration-prototype CO2-laser heterodyne spectrometer operating at 9-12 microns and suitable for long-term space missions is described and illustrated with extensive diagrams, drawings, photographs, and graphs of test performance data. The spectrometer has total volume 0.63 cu m, mass 30 kg, and power requirement 60-70 W, compatible with miniature-class Space Shuttle experiment payload specifications. It comprises three modules: (1) an optical front end with reflecting optics, a 2-GHz BW HgCdTe photomixer, and a 0-2-GHz 40-dB RF preamplifier; (2) a local oscillator with an RF-excited waveguide CO2 laser, a 75-percent-efficiency RF amplifier, a stepper-driven grating mode selector, and an etalon stabilized for over 30,000 h of use; and (3) an RF-filter-bank spectral-line receiver with a 25-MHz RF channel, 1.6-GHz IF spectral coverage, onboard instrument control, a serial link to the host computer, and highly integrated design.

Paper Details

Date Published: 1 July 1990
PDF: 10 pages
Proc. SPIE 1235, Instrumentation in Astronomy VII, (1 July 1990); doi: 10.1117/12.19156
Show Author Affiliations
David Alan Glenar, NASA/Goddard Space Flight Ctr. (United States)
M. J. Mumma, NASA/Goddard Space Flight Ctr. (United States)
Theodore Kostiuk, NASA/Goddard Space Flight Ctr. (United States)
H. Huffman, NASA/Goddard Space Flight Ctr. (United States)
John J. Degnan, NASA/Goddard Space Flight Ctr. (United States)
Hemant H. Dave, Applied Research Corp. (India)
Urs E. Hochuli, Univ. of Maryland (United States)
Paul R. Haldemann, Univ. of Maryland (United States)

Published in SPIE Proceedings Vol. 1235:
Instrumentation in Astronomy VII
David L. Crawford, Editor(s)

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