High resolution solar spectrometer system for measuring atmospheric constituents

Details High resolution solar spectrometer system for measuring atmospheric constituents High resolution solar spectrometer system for measuring atmospheric constituents

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apopt..29.1520m&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 29, April 1, 1990, p. 1520-1525. Research supported by NSF and NASA.

Physics

Optics

17

Atmospheric Composition, Balloon-Borne Instruments, Line Spectra, Michelson Interferometers, Solar Spectrometers, Absorption Spectra, High Resolution, Infrared Interferometers, Telemetry

Scientific paper

A mid-IR Michelson interferometer capable of obtaining 0.002/cm resolution solar spectra has been developed for balloon use. The interferometer is based on the Bomem self-aligning instrument, and is equipped with a solar tracking system, telemetry, and recording systems, as well as temperature control and gondola orientation. The interferometer has made two successful flights in the 7-14-micron interval up to 40 km. The basic systems are described and sample spectra are presented.

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