Stilbs to Foot-Lamberts
Snapshot
1 Stilbs equals 2,918.63508 Foot-Lamberts.
- Reference basis: This conversion uses fixed luminance constants anchored to candela per square meter.
- Example: For 5 Stilbs, the result equals 14,593.175398 Foot-Lamberts.
Interactive conversion
Converter Calculator
Decimals: 1.5 or 1,5. Fractions: 1/2. Scientific notation: 1e3. Write 1000 without grouping separators.
2,918.63508 Foot-Lamberts (fL)
SwitchAPI and AI agent access
Stilbs to Foot-Lamberts.
Machine-readable identifiers
- Conversion family
photometry-imaging- Source unit
stilbs- Target unit
foot_lamberts
Use these identifiers in the API request. Sources and model limits also apply to software clients.
Example API request and response
POST /api/v1/convertRequest
{
"family": "photometry-imaging",
"value": 1,
"from": "stilbs",
"to": "foot_lamberts"
}Essential response
{
"ok": true,
"conversion": {
"family": "photometry-imaging",
"value": 1,
"from": "stilbs",
"to": "foot_lamberts",
"result": {
"raw": 2918.63507963,
"display": "2,918.63508"
},
"canonicalPath": "/photometry-imaging/stilbs-to-foot-lamberts/"
}
}Explanation
The converter converts stilbs into foot-lamberts by normalizing both luminance units through candela per square meter. Formula: fL = sb × 2918.63507963. That keeps the snapshot, calculator, common values, and mirror page aligned on one luminance basis.
This is useful for display brightness checks, projection calibration, and imaging workflows where legacy photometric units and modern cd/m²-based measurements need to match cleanly.
Common Conversion Values
| Stilbs (sb) | Foot-Lamberts (fL) |
|---|---|
| 1 | 2,918.63508 |
| 5 | 14,593.175398 |
| 10 | 29,186.350796 |
| 25 | 72,965.876991 |
| 50 | 145,931.753982 |
| 100 | 291,863.507963 |
| 250 | 729,658.769908 |
| 500 | 1,459,317.539815 |
| 1000 | 2,918,635.07963 |
Questions & answers
Frequently Asked Questions
Why is Stilbs to Foot-Lamberts useful in display and projection work?
This route is useful when comparing modern display-brightness values with legacy luminance units used in cinema, projection, calibration, and older imaging references.
When would I convert stilbs to foot-lamberts?
This route is useful when comparing modern display-brightness values with legacy luminance units used in projection, cinema, and older photometric references.
How do I reverse Stilbs to Foot-Lamberts?
Use the mirror Foot-Lamberts to Stilbs route; it applies the inverse relationship with the same cd/m²-based luminance assumptions.