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Lambert (unit)

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The lambert (symbol L, la [ citation needed ] or Lb [ citation needed ] ) is a non- SI metric unit of luminance named for Johann Heinrich Lambert (1728?1777), a Swiss mathematician, physicist and astronomer. A related unit of luminance, the foot-lambert , is used in the lighting, cinema and flight simulation industries. The SI unit is the candela per square metre (cd/m 2 ).

Definition [ edit ]

1 lambert (L) = candela per square centimetre (0.3183 cd/cm 2 ) or cd  m ?2

Units of luminance
cd/m 2 ( SI unit)
≡ nit ≡ lm/m 2 /sr
stilb (sb) ( CGS unit)
≡ cd/cm 2
apostilb (asb)
≡ blondel
bril skot (sk) lambert (L) foot-lambert (fL)
= 1 ⁄ π cd/ft 2
1 cd/m 2 = 1 10 ?4 π
? 3.142
10 7 π
? 3.142 × 10 7
10 3 π
? 3.142 × 10 3
10 ?4 π
? 3.142 × 10 ?4
0.3048 2 π
? 0.2919
1 sb = 10 4 1 10 4 π
? 3.142 × 10 4
10 11 π
? 3.142 × 10 11
10 7 π
? 3.142 × 10 7
π
? 3.142
30.48 2 π
? 2919
1 asb = 1 ⁄ π
? 0.3183
10 ?4 π
? 3.183 × 10 ?5
1 10 7 10 3 10 ?4 0.3048 2
? 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 0.3048 2 × 10 ?7
? 9.290 × 10 ?9
1 sk = 10 ?3 π
? 3.183 × 10 ?4
10 ?7 π
? 3.183 × 10 ?8
10 ?3 10 4 1 10 ?7 0.3048 2 × 10 ?3
? 9.290 × 10 ?5
1 L = 10 4 π
? 3183
1 ⁄ π
? 0.3183
10 4 10 11 10 7 1 0.3048 2 × 10 4
? 929.0
1 fL = 1 ⁄ 0.3048 2 π
? 3.426
1 ⁄ 30.48 2 π
? 3.426 × 10 ?4
1 ⁄ 0.3048 2
? 10.76
10 7 ⁄ 0.3048 2
? 1.076 × 10 8
10 3 ⁄ 0.3048 2
? 1.076 × 10 4
10 ?4 ⁄ 0.3048 2
? 1.076 × 10 ?3
1

See also [ edit ]

Other units of luminance:

Quantity Unit Dimension
[nb 1]
Notes
Name Symbol [nb 2] Name Symbol
Luminous energy Q v [nb 3] lumen second lm ?s T ? J The lumen second is sometimes called the talbot .
Luminous flux , luminous power Φ v [nb 3] lumen (= candela steradian ) lm (= cd?sr) J Luminous energy per unit time
Luminous intensity I v candela (= lumen per steradian) cd (= lm/sr) J Luminous flux per unit solid angle
Luminance L v candela per square metre cd/m 2 (= lm/(sr?m 2 )) L ?2 ? J Luminous flux per unit solid angle per unit projected source area. The candela per square metre is sometimes called the nit .
Illuminance E v lux (= lumen per square metre) lx (= lm/m 2 ) L ?2 ? J Luminous flux incident on a surface
Luminous exitance , luminous emittance M v lumen per square metre lm/m 2 L ?2 ? J Luminous flux emitted from a surface
Luminous exposure H v lux second lx?s L ?2 ? T ? J Time-integrated illuminance
Luminous energy density ω v lumen second per cubic metre lm?s/m 3 L ?3 ? T ? J
Luminous efficacy (of radiation) K lumen per watt lm/ W M ?1 ? L ?2 ? T 3 ? J Ratio of luminous flux to radiant flux
Luminous efficacy (of a source) η [nb 3] lumen per watt lm/ W M ?1 ? L ?2 ? T 3 ? J Ratio of luminous flux to power consumption
Luminous efficiency , luminous coefficient V 1 Luminous efficacy normalized by the maximum possible efficacy
See also:
  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. ^ a b c Alternative symbols sometimes seen: W for luminous energy, P or F for luminous flux, and ρ for luminous efficacy of a source.

References [ edit ]