Paper
26 September 1977 Reducing Optical Noise
Clifford J. Chocol, Jack F. Wade
Author Affiliations +
Proceedings Volume 0107, Stray Light Problems in Optical Systems; (1977) https://doi.org/10.1117/12.964606
Event: 1977 SPIE/SPSE Technical Symposium East, 1977, Reston, United States
Abstract
Light suppression in optical instruments has improved significantly in the last several years. These improvements can be attributed directly to three previous developments: optical computer programs, low reflecting surfaces and more efficient baffle edges. In 1968 a new electro-chemical process was developed, which with subsequent refinement, exhibited a reflectance of about 0.57 over the visible (Figure 1) and infrared spectrum (8-14 μm). Several years later a method was devised to fabricate baffle edges which when subjected to the electro-chemical process, produced edges 8 to 10 times more efficient (Figure 2) than the previous state-of-the-art. With refinement in the computer programs and experimentally obtained data on surfaces and edges, light shades were designed and tested which exhibited an improvement over previous light shades by an order of magnitude. This combination of computer program and physical properties improvements has enabled us to improve instruments performance significantly by reducing the largest source of noise, i.e., stray light.
© (1977) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Clifford J. Chocol and Jack F. Wade "Reducing Optical Noise", Proc. SPIE 0107, Stray Light Problems in Optical Systems, (26 September 1977); https://doi.org/10.1117/12.964606
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KEYWORDS
Software

Reflectivity

Coating

Data modeling

Stray light

Signal to noise ratio

Reflection

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