Expressions relating the roughness of a plane surface to its specular reflectance at normal incidence are presented and are verified experimentally. The expressions are valid for the case when the root mean square surface roughness is small compared to the wavelength of light. If light of a sufficiently long wavelength is used, the decrease in measured specular reflectance due to surface roughness is a function only of the root mean square height of the surface irregularities. Long-wavelength specular reflectance measurements thus provide a simple and sensitive method for accurate measurement of surface finish. This method is particularly useful for surface finishes too fine to be measured accurately by conventional tracing instruments. Surface roughness must also be considered in precise optical measurements. For example, a non-negligible systematic error in specular reflectance measurements will be made even if the root mean square surface roughness is less than 0.01 wavelength. The roughness of even optically polished surfaces may thus be important for measurements in the visible and ultraviolet regions of the spectrum.
[1]
F W Preston,et al.
The structure of abraded glass surfaces
,
1922
.
[2]
J. Guild.
An optical smoothness-meter for evaluating the surface finish of metals
,
1940
.
[3]
A glossmeter for smoothness comparisons of machine-finished surfaces
,
1946
.
[4]
W. Koehler.
Multiple-Beam Fringes of Equal Chromatic Order. Part VII. Mechanism of Polishing Glass*
,
1953
.
[5]
J. Halling.
A reflectometer for the assessment of surface texture
,
1954
.
[6]
W. White,et al.
Multiple-Beam Fringes of Equal Chromatic Order. Part VI. Method of Measuring Roughness*
,
1955
.
[7]
H. Hasunuma,et al.
On the Sheen Gloss
,
1956
.
[8]
W. Middleton,et al.
Colors Produced by Reflection at Grazing Incidence from Rough Surfaces
,
1957
.
[9]
H. E. Bennett,et al.
Precision Measurement of Absolute Specular Reflectance with Minimized Systematic Errors
,
1960
.