Paper
7 September 2013 Incorporating skew into RMS surface roughness probability distributions
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Abstract
Characterizing surface roughness is important for predicting optical performance. Typically, this is accomplished by taking multiple statistically independent measurements and averaging. But, this approach assumes that the statistical distribution of the roughness has a Gaussian (normal) probability distribution. Our analysis shows that this assumption is wrong. Real data acquired from two different sets of telescope optics indicates that roughness of highly polished surfaces is skewed and is best described by a largest extreme value probability (LEV) distribution. Assuming a normal distribution and simply averaging overestimates the most probable surface roughness and could result in the expenditure of unnecessary polishing effort.
© (2013) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mark T. Stahl and H. Philip Stahl "Incorporating skew into RMS surface roughness probability distributions", Proc. SPIE 8838, Optical Manufacturing and Testing X, 883814 (7 September 2013); https://doi.org/10.1117/12.2024883
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Cited by 1 scholarly publication.
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KEYWORDS
Statistical analysis

Surface roughness

James Webb Space Telescope

Polishing

Surface finishing

Manufacturing

Telescopes

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