NASA applications for acousto-optic spectrometers

Details NASA applications for acousto-optic spectrometers NASA applications for acousto-optic spectrometers

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984spie..477..128c&link_type=abstract

IN: Optical technology for microwave applications; Proceedings of the Meeting, Arlington, VA, May 1, 2, 1984 (A86-15251 04-33).

Physics

Optics

Acousto-Optics, Heterodyning, Spaceborne Telescopes, Spectrometers, Submillimeter Waves, Bandpass Filters, High Resolution, Molecular Spectra, Nasa Programs, Signal To Noise Ratios

Scientific paper

Small, compact, and rugged IF spectrometers are needed in high resolution heterodyne receivers designed for a new generation of space-borne telescopes planned for the next decade. Acousto-optic Spectrometers (AOS) promise to provide the necessary bandwidth and resolution in a package which is compact, power efficient, and ruggedized for space applications. Sensitivity, linearity, and stability are the primary goals of an astronomical receiver and these features must be demonstrated in order for an AOS to be accepted in place of more conventional RF or digital technology.

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