Understanding Stilbs to Foot-Lamberts Conversion
The stilb (sb) is a CGS luminance unit equal to one candela per square centimeter. The foot-lambert (fL) is an imperial luminance unit equal to (1/π) candela per square foot, still used in cinema projection and display calibration to specify screen brightness. Converting stilbs to foot-lamberts is common when bright emitter data must be expressed in the units projectionists and AV engineers work with.
Conversion Formula
To convert stilbs to foot-lamberts, multiply by this factor:
Step-by-Step Example
Convert 25 stilbs to foot-lamberts.
How to Convert Stilbs to Foot-Lamberts
Express a bright-surface luminance in the imperial unit used for screen calibration.
- Take the stilb value: For example, 25 sb.
- Multiply by 2918.635: This factor combines the area change and the 1/π foot-lambert definition.
- Compute: .
- State the result: 25 stilbs equals about 72,965.9 fL.
stilbs to foot-lamberts conversion table
| stilbs (sb) | foot-lamberts (fL) |
|---|---|
| 0 | 0 |
| 1 | 2918.635 |
| 2 | 5837.27 |
| 3 | 8755.905 |
| 4 | 11674.54 |
| 5 | 14593.18 |
| 6 | 17511.81 |
| 7 | 20430.45 |
| 8 | 23349.08 |
| 9 | 26267.72 |
| 10 | 29186.35 |
| 15 | 43779.53 |
| 20 | 58372.7 |
| 25 | 72965.88 |
| 30 | 87559.05 |
| 40 | 116745.4 |
| 50 | 145931.8 |
| 60 | 175118.1 |
| 70 | 204304.5 |
| 80 | 233490.8 |
| 90 | 262677.2 |
| 100 | 291863.5 |
| 150 | 437795.3 |
| 200 | 583727 |
| 250 | 729658.8 |
| 300 | 875590.5 |
| 400 | 1167454 |
| 500 | 1459318 |
| 600 | 1751181 |
| 700 | 2043045 |
| 800 | 2334908 |
| 900 | 2626772 |
| 1000 | 2918635 |
| 2000 | 5837270 |
| 3000 | 8755905 |
| 4000 | 11674540 |
| 5000 | 14593180 |
| 10000 | 29186350 |
| 25000 | 72965880 |
| 50000 | 145931800 |
| 100000 | 291863500 |
| 250000 | 729658800 |
| 500000 | 1459318000 |
| 1000000 | 2918635000 |
What is the stilb?
The stilb is a CGS unit of luminance, describing the brightness of a surface in terms of luminous intensity per unit area. It was widely used in older photometric literature before the SI candela per square metre became standard.
Definition
One stilb is one candela per square centimetre. Since there are ten thousand square centimetres in a square metre, the stilb is a large unit relative to the SI luminance unit.
Exactly, .
Origin and History
The stilb was introduced by the French physicist André Blondel around 1920, its name taken from the Greek stilbein, "to glitter." It belonged to the centimetre–gram–second system and was used chiefly in continental Europe.
Law and Notable Facts
The stilb is not part of the SI and has largely fallen out of use in favour of the candela per square metre. Because it references the square centimetre, a single stilb represents a very bright surface: the sun's disc at the horizon is on the order of a few hundred stilbs.
Real-World Examples and Conversions
- A frosted incandescent lamp surface: a few stilbs.
- The sun's disc viewed from Earth: roughly 160,000 cd/m², or about 16 stilbs.
- .
- .
What is the Foot-Lambert?
The foot-lambert is a non-SI unit of luminance, expressing the brightness of a surface as seen by an observer. It remains widely used in the cinema, projection, and display industries in the United States, where screen brightness is often specified in foot-lamberts.
Definition
The foot-lambert is defined so that a perfectly diffusing (Lambertian) surface emitting or reflecting a total luminous flux of one lumen per square foot has a luminance of one foot-lambert.
Equivalently, . As with the lambert, the factor of arises from the cosine emission geometry of a Lambertian source. Because one square foot equals , the conversion follows directly: .
Origin and History
The foot-lambert is the imperial-unit counterpart of the lambert, both descending from Johann Heinrich Lambert's foundational photometry. It became entrenched in mid-20th-century American engineering practice, particularly in cinema, where SMPTE standards long specified projected picture brightness in foot-lamberts.
Law and Notable Facts
The foot-lambert is not an SI unit, but it persists in professional standards. SMPTE recommends an open-gate (unmodulated) screen luminance of 14 fL (≈ 48 cd/m²) for film projection and 16 fL peak white for digital cinema in a dark theater. HDR home displays, by contrast, target hundreds to over a thousand cd/m².
Real-World Examples and Conversions
- 14 foot-lamberts (SMPTE film reference) ≈ 47.97 cd/m².
- 1 foot-lambert ≈ 3.42626 cd/m² ≈ 0.001076 lambert.
- A typical office display of 250 cd/m² is about 73 foot-lamberts.
- 1 lambert ≈ 929.03 foot-lamberts.
Frequently Asked Questions
How many foot-lamberts equal one stilb?
One stilb equals 2,918.635 foot-lamberts.
How do I convert foot-lamberts back to stilbs?
Multiply the foot-lambert value by 0.0003426259. So 2,918.635 fL equals 1 sb.
Where are foot-lamberts used?
Foot-lamberts are standard in cinema and home-theater calibration; SMPTE recommends about 14 fL for film projection on screen.
Why does the foot-lambert include a 1/π factor?
The foot-lambert is defined so that a perfectly diffuse surface emitting one lumen per square foot has a luminance of one fL, which introduces the 1/π factor relative to candela-per-area units.
What is 2 stilbs in foot-lamberts?
Multiply 2 by 2,918.635 to get 5,837.27 fL.
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Complete stilbs conversion table
| Unit | Result |
|---|---|
| candelas per square metre (cd/m2) | 10000 cd/m2 |
| nits (nt) | 10000 nt |
| apostilbs (asb) | 31415.93 asb |
| lamberts (L) | 3.141593 L |
| foot-lamberts (fL) | 2918.635 fL |