High resolution Michelson interferometer for airborne infrared astronomical observations. I - Concept and performance

Astronomy and Astrophysics – Astronomy

Scientific paper

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Airborne Equipment, Computer Techniques, High Resolution, Infrared Spectroscopy, Michelson Interferometers, Telescopes, Calibrating, Data Management, Display Devices, H Ii Regions, H Lines, Infrared Astronomy, Minicomputers, Spectral Resolution

Scientific paper

A Michelson interferometer has been built for use with the 91-cm telescope on NASA's Gerard P. Kuiper Airborne Observatory primarily to measure IR line emission from H II regions. Operation is in the rapid scan mode, and the achievable resolution is 0.02/cm in the wavelength range from 10 to around 300 microns. A minicomputer is used to provide on-line spectrum displays and to control and monitor the instrument performance. The design and use of the instrument is discussed, and a comparison is made between the theoretical performance and that actually achieved on the first flights when measurements of line emission from the Orion nebula and from the atmosphere were made.

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