Editing Mirror (section)

== Manufacturing ==
[[File:Hubble mirror polishing.jpg|thumb|Polishing the primary mirror for the [[Hubble Space Telescope]]. A deviation in the surface quality of approximately 4λ resulted in poor images initially, which was eventually compensated for using [[Corrective Optics Space Telescope Axial Replacement|corrective optics]].]]

Mirrors are usually manufactured by either polishing a naturally reflective material, such as speculum metal, or by applying a [[silvering|reflective coating]] to a suitable polished [[substrate (materials science)|substrate]].<ref name=lanz2012/>

In some applications, generally those that are cost-sensitive or that require great durability, such as for mounting in a prison cell, mirrors may be made from a single, bulk material such as polished metal. However, metals consist of small crystals (grains) separated by grain boundaries that may prevent the surface from attaining optical smoothness and uniform reflectivity.<ref name=pulk1999/>{{rp|p.2,8}}

===Coating===
====Silvering====
{{main|silvering}}
The coating of glass with a reflective layer of a metal is generally called "[[silvering]]", even though the metal may not be silver. Currently the main processes are [[electroplating]], "wet" [[electroless plating|chemical deposition]], and [[vacuum deposition]].<ref name=pulk1999/> Front-coated metal mirrors achieve reflectivities of 90–95% when new.

====Dielectric coating====
Applications requiring higher reflectivity or greater durability, where wide [[bandwidth (signal processing)|bandwidth]] is not essential, use [[dielectric mirror|dielectric coatings]], which can achieve reflectivities as high as 99.997% over a limited range of wavelengths. Because they are often chemically stable and do not conduct electricity, dielectric coatings are almost always applied by methods of vacuum deposition, and most commonly by evaporation deposition. Because the coatings are usually transparent, absorption losses are negligible. Unlike with metals, the reflectivity of the individual dielectric-coatings is a function of [[Snell's law]] known as the [[Fresnel equations]], determined by the difference in [[refractive index]] between layers. Therefore, the thickness and index of the coatings can be adjusted to be centered on any wavelength. Vacuum deposition can be achieved in a number of ways, including sputtering, evaporation deposition, arc deposition, reactive-gas deposition, and ion plating, among many others.<ref name=pulk1999/>{{rp|p.103,107}}

===Shaping and polishing===
====Tolerances====
Mirrors can be manufactured to a wide range of [[engineering tolerance]]s, including [[reflectivity]], surface quality, [[surface roughness]], or [[Transmittance|transmissivity]], depending on the desired application. These tolerances can range from wide, such as found in a normal household-mirror, to extremely narrow, like those used in lasers or telescopes. Tightening the tolerances allows better and more precise imaging or beam transmission over longer distances. In imaging systems this can help reduce anomalies ([[Artifact (error)|artifacts]]), distortion or blur, but at a much higher cost. Where viewing distances are relatively close or high precision is not a concern, wider tolerances can be used to make effective mirrors at affordable costs.