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Blue-green Fraunhofer-wavelength atomic filters

Jerry A. Gelbwachs

Published Jan 1, 1991• 0 citations
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The atomic resonance filter (ARF) is art ultra- high-Q (105–106) optical filter that is isotropic and insensitive to environmental factors and possesses a 180° acceptance angle.1 We are developing a novel ARF for satellite applications. Our filter operates in a Fraunhofer dip in the solar spectrum, thereby offering the key advantage of reduced solar background noise. Other important operational characteristics of the filter are: a projected conversion efficiency of blue-green light into the wavelength-shifted output light of ~90%, a 10-ns response time, and an output in the near UV, a spectral region that is efficiently detected by commercial large-area long-lived photomultiplier tubes.

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We describe what is to our knowledge the first experimental demonstration of internal wavelength conversion in the metastable Mg atomic filter. The filter operates at a Fraunhofer line, thereby offering intrinsic solar background rejection. Incoming green Fraunhofer photons (518 nm) are absorbed by metastable Mg atoms in an oven cell and are converted into UV (384-nm) photons. We observed a green-to-UV conversion efficiency of greater than 50%.

Optics Letters•Jul 15, 1989•19 citations
The atomic resonance filter (ARF) is art ultra- high-Q (105–106) optical filter that is isotropic and insensitive to environmental factors and possesses a 180° acceptance angle.1 We are developing a novel ARF for satellite applications. Our filter operates in a Fraunhofer dip in the solar spectrum, thereby offering the key advantage of reduced solar background noise. Other important operational characteristics of the filter are: a projected conversion efficiency of blue-green light into the wavelength-shifted output light of ~90%, a 10-ns response time, and an output in the near UV, a spectral region that is efficiently detected by commercial large-area long-lived photomultiplier tubes.