Foot-Lamberts to Apostilbs
Snapshot
1 Foot-Lamberts equals 10.76391 Apostilbs.
- Reference basis: This conversion uses fixed luminance constants anchored to candela per square meter.
- Example: For 5 Foot-Lamberts, the result equals 53.819552 Apostilbs.
Interactive conversion
Converter Calculator
Decimals: 1.5 or 1,5. Fractions: 1/2. Scientific notation: 1e3. Write 1000 without grouping separators.
10.76391 Apostilbs (asb)
SwitchAPI and AI agent access
Foot-Lamberts to Apostilbs.
Machine-readable identifiers
- Conversion family
photometry-imaging- Source unit
foot_lamberts- Target unit
apostilbs
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": "foot_lamberts",
"to": "apostilbs"
}Essential response
{
"ok": true,
"conversion": {
"family": "photometry-imaging",
"value": 1,
"from": "foot_lamberts",
"to": "apostilbs",
"result": {
"raw": 10.7639104166,
"display": "10.76391"
},
"canonicalPath": "/photometry-imaging/foot-lamberts-to-apostilbs/"
}
}Explanation
The converter converts foot-lamberts into apostilbs by normalizing both luminance units through candela per square meter. Formula: asb = fL × 10.7639104166. 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
| Foot-Lamberts (fL) | Apostilbs (asb) |
|---|---|
| 1 | 10.76391 |
| 5 | 53.819552 |
| 10 | 107.639104 |
| 25 | 269.09776 |
| 50 | 538.195521 |
| 100 | 1,076.391042 |
| 250 | 2,690.977604 |
| 500 | 5,381.955208 |
| 1000 | 10,763.910417 |
Questions & answers
Frequently Asked Questions
Why is Foot-Lamberts to Apostilbs 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 foot-lamberts to apostilbs?
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 Foot-Lamberts to Apostilbs?
Use the mirror Apostilbs to Foot-Lamberts route; it applies the inverse relationship with the same cd/m²-based luminance assumptions.