Paper
9 August 1988 Fractal Surface Finish
Eugene L. Church
Author Affiliations +
Abstract
Surface finish measurements are usually fitted to models of the finish correlation function which are parametrized in terms of root-mean-square roughnesses, σ, and correlation lengths, l. Highly finished optical surfaces, however, are frequently better described by fractal models, which involve inverse power-law spectra and are parametrized by spectral strengths, Kn, and spectral indices, n. Analyzing measurements of fractal surfaces in terms of σ and l gives results which are not intrinsic surface parameters but which depend on the bandwidth parameters of the measurement process used. This paper derives expressions for these pseudo-parameters and discusses the errors involved in using them for the characterization and specification of surface finish.
© (1988) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Eugene L. Church "Fractal Surface Finish", Proc. SPIE 0830, Grazing Incidence Optics for Astronomical and Laboratory Applications, (9 August 1988); https://doi.org/10.1117/12.942165
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Fractal analysis

Surface finishing

Correlation function

Scattering

Scatter measurement

Astronomical imaging

Astronomy

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