422.7-nm atomic filter with superior solar background rejection
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Updated: Jun 20, 2026

Rejection of Fluorescence Background in Resonance and Spontaneous Raman Microspectroscopy
Published on: May 18, 2011
1Chemistry and Physics Laboratory, The Aerospace Corporation, M2/253, P.O. Box 92957, Los Angeles, California 90009, USA.
Abstract:
A novel atomic resonance filter with powerful solar background rejection is proposed. The filter wavelength matches the g Fraunhofer line at 422.7 nm. Atomic filtering occurs within the singlet manifold of neutral calcium. Superior sunlight discrimination arises mainly from two factors: overlay with an intense Fraunhofer line and signal levels devoid of fine and hyperfine structures. The new filter should exhibit high throughput and low noise.
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