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There is a fundamental distinction between household mirrors and optical mirrors; the latter is coated on the front surface instead of the back. This requirement means that for optical applications, a front-surface mirror is essential. Although typically housed within enclosures, the reflective surface is still susceptible to environmental degradation. Creating a robust front-surface mirror capable of withstanding wear and being easily cleaned is vital in mirror technology.
The substrate surface of a mirror should have a flat and smooth profile. Flatness is generally specified in terms of how many wavelengths of light the surface diverges from perfect flatness. For many cases, glass can be flattened to a few wavelengths of visible light. However, the most demanding applications require that the surface be flat to less than a quarter of a wavelength. Surface quality, or smoothness, is assessed based on the presence of scratches and digs post-polishing. A scratch/dig specification of 80/50 is common, while a specification of 20/10 offers higher transparency but at a greater cost.
Certain applications require a mirror's thermal conductance to be factored in. Metal substrates are often used in these cases, as they are generally more conductive than glass. Optical-quality metal surfaces can be crafted through polishing or single-point diamond turning. Common options include copper and aluminum, while beryllium is occasionally selected for its lightweight and rigidity—though it is notably toxic. In scenarios utilizing metal substrates, coatings serve to enhance reflectance while providing durability and scratch resistance.
Metal Mirror Coatings
The simplest and most widespread mirror coating involves a thin layer of metal. A 100-nm layer of aluminum or silver produces an excellent reflector in the visible spectrum. Aluminum reflects approximately 90% of light in this range, while silver achieves about 95%. The reflectivity of a metal mirror can be determined via the metal's index of refraction (n) and extinction coefficient (k). Reflectance is defined as follows:
An extensive compilation of n and k values across various wavelengths and metals is readily accessible. Table 1 presents an abridged selection, detailing data for ultraviolet (0.2 and 0.3 µm), visible (0.4 to 0.7 µm), and infrared wavelengths (1 to 10 µm). Metals characterized by k >> n tend to exhibit shininess, whereas those with k ≤ n ≤ 3 appear gray. For example, silver has n = 0.13 and k = 2.92 at 0.5 µm, making it shiny, while tungsten has n = 3.4 and k = 2.69, rendering it less shiny. As the wavelength trends into the IR region, both n and k increase, which leads to heightened reflectivity in that spectral region.
TABLE 1.
n AND k FOR SELECTED METALS
Wavelength (µm):
0.2
0.3
0.4
0.5
0.6
0.7
1.0
2.0
4.0
10.0
Aluminum* n:
k:
0.12
2.30
0.28
3.61
0.49
4.86
0.77
6.08
1.20
7.26
1.83
8.31
1.35
9.58
2.15
20.7
6.43
39.8
25.3
89.8
Beryllium n:
k:
0.84
2.52
2.42
3.09
2.89
3.13
3.25
3.17
3.43
3.18
3.47
3.25
3.28
3.87
2.44
7.61
2.38
16.7
8.3
41.0
Chromium n:
k:
0.89
1.69
0.98
2.67
1.50
3.59
2.61
4.45
3.43
4.37
3.84
4.37
4.50
4.28
4.01
6.31
3.08
13.7
14.2
27.5
For applications requiring higher durability, less shiny metals can suffice. For instance, dental mirrors utilize rhodium and rearview mirrors in vehicles use chromium.
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