Paper
14 September 1994 Fabry-Perot techniques for observation of diffuse atmospheric sources
Ted B. Williams
Author Affiliations +
Abstract
An imaging Fabry-Perot interferometer combined with a CCD detector can provide extremely high sensitivity for the detection of diffuse atmospheric spectral emission features. We present a description of the theory and operation of a modern servo-stabilized Fabry-Perot etalon, derive the limiting sensitivity for typical optical configurations, and present astronomical observations of faint, diffuse emission line sources as examples of the technique. We show that sources with intensity as faint as 10-2 Rayleigh can be detected with a few hours of integration.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Ted B. Williams "Fabry-Perot techniques for observation of diffuse atmospheric sources", Proc. SPIE 2282, Ultraviolet Technology V, (14 September 1994); https://doi.org/10.1117/12.186602
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KEYWORDS
Fabry–Perot interferometers

Sensors

Telescopes

Imaging systems

Ultraviolet radiation

Spectral resolution

Astronomy

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