Stilb (unit)

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The stilb (sb) is the CGS unit of luminance for objects that are not self-luminous. It is equal to one candela per square centimeter or 104 nits (candelas per square meter). The name was coined by the French physicist André Blondel around 1920.[1] It comes from the Greek word stilbein (στίλβειν), meaning 'to glitter'.

It was in common use in Europe up to World War I. In North America self-explanatory terms such as candle per square inch and candle per square meter were more common.[2] The unit has since largely been replaced by the SI unit: candela per square meter. The current national standard for SI in the United States discourages the use of the stilb.[3]

Unit conversion

More information cd/m2 (SI unit) ≡ nit ≡ lm/m2/sr, stilb (sb) (CGS unit) ≡ cd/cm2 ...
Units of luminance
cd/m2 (SI unit)
≡ nit ≡ lm/m2/sr
stilb (sb) (CGS unit)
≡ cd/cm2
apostilb (asb)
≡ blondel
bril skot (sk) lambert (L) foot-lambert (fL)
= 1 π cd/ft2
1 cd/m2 = 1 10−4 π
≈ 3.142
107 π
≈ 3.142×107
103 π
≈ 3.142×103
10−4 π
≈ 3.142×10−4
0.30482 π
≈ 0.2919
1 sb = 104 1 104 π
≈ 3.142×104
1011 π
≈ 3.142×1011
107 π
≈ 3.142×107
π
≈ 3.142
30.482 π
≈ 2919
1 asb = 1 π
≈ 0.3183
10−4 π
≈ 3.183×10−5
1 107 103 10−4 0.30482
≈ 0.09290
1 bril = 10−7 π
≈ 3.183×10−8
10−11 π
≈ 3.183×10−12
10−7 1 10−4 10−11 0.30482×10−7
≈ 9.290×10−9
1 sk = 10−3 π
≈ 3.183×10−4
10−7 π
≈ 3.183×10−8
10−3 104 1 10−7 0.30482×10−3
≈ 9.290×10−5
1 L = 104 π
≈ 3183
1 π
≈ 0.3183
104 1011 107 1 0.30482×104
≈ 929.0
1 fL = 1 0.30482 π
≈ 3.426
1 30.482 π
≈ 3.426×10−4
1 0.30482
≈ 10.76
107 0.30482
≈ 1.076×108
103 0.30482
≈ 1.076×104
10−4 0.30482
≈ 1.076×10−3
1
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More information Quantity, Unit ...
Quantity Unit Dimension
[nb 1]
Notes
Name Symbol[nb 2] Name Symbol
Luminous energy Qv[nb 3] lumen second lm⋅s TJ The lumen second is sometimes called the talbot.
Luminous flux, luminous power Φv[nb 3] lumen (= candela steradian) lm (= cd⋅sr) J Luminous energy per unit time
Luminous intensity Iv candela (= lumen per steradian) cd (= lm/sr) J Luminous flux per unit solid angle
Luminance Lv candela per square metre cd/m2 (= lm/(sr⋅m2)) L−2J Luminous flux per unit solid angle per unit projected source area. The candela per square metre is sometimes called the nit.
Illuminance Ev lux (= lumen per square metre) lx (= lm/m2) L−2J Luminous flux incident on a surface
Luminous exitance, luminous emittance Mv lumen per square metre lm/m2 L−2J Luminous flux emitted from a surface
Luminous exposure Hv lux second lx⋅s L−2TJ Time-integrated illuminance
Luminous energy density ωv lumen second per cubic metre lm⋅s/m3 L−3TJ
Luminous efficacy (of radiation) K lumen per watt lm/W M−1L−2T3J Ratio of luminous flux to radiant flux
Luminous efficacy (of a source) η[nb 3] lumen per watt lm/W M−1L−2T3J Ratio of luminous flux to power consumption
Luminous efficiency, luminous coefficient V 1 Luminous efficacy normalized by the maximum possible efficacy
See also:
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  1. The symbols in this column denote dimensions; "L", "T" and "J" are for length, time and luminous intensity respectively, not the symbols for the units litre, tesla and joule.
  2. Standards organizations recommend that photometric quantities be denoted with a subscript "v" (for "visual") to avoid confusion with radiometric or photon quantities. For example: USA Standard Letter Symbols for Illuminating Engineering USAS Z7.1-1967, Y10.18-1967
  3. Alternative symbols sometimes seen: W for luminous energy, P or F for luminous flux, and ρ for luminous efficacy of a source.

See also

References

Further reading

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