Optics and transmitter parameters, by model
Divergence, receiver aperture, pulse energy and update rate for 50 models — the four numbers that decide the photon budget, plus the spot diameter they produce at 1 km so the effect of divergence is visible rather than theoretical.
The table
| Model | Wavelength | Divergence | Spot at 1 km | Receiver / lens | Pulse energy | Update rate |
|---|---|---|---|---|---|---|
| LRF0815C | 1535 nm | 0.3 mrad | 0.3 m | 12 mm | 300 µJ | 10 Hz |
| LRF0612C | 1535 nm | 0.3 mrad | 0.3 m | 12 mm | 200 µJ | 10 Hz |
| LRF0816C | 1535 nm | 0.3 mrad | 0.3 m | 12 mm | 300 µJ | 10 Hz |
| LRF1017C | 1.54 µm | 0.3 mrad | 0.3 m | 12 mm | 300 µJ | 10 Hz |
| LRF1221C | 1.54 µm | 0.3 mrad | 0.3 m | 12 mm | 300 µJ | 10 Hz |
| LRF1222C | 1.54 µm | 0.3 mrad | 0.3 m | 16.5 mm | 300 µJ | 10 Hz |
| LRF1525C | 1.54 µm | 0.3 mrad | 0.3 m | 15 mm | 500 µJ | 10 Hz |
| LRF1829C | 1535 nm | 0.3 mrad | 0.3 m | 18 mm | 500 µJ | 10 Hz |
| LRF1830C | 1.54 µm | 0.3 mrad | 0.3 m | 18 mm | 500 µJ | 10 Hz |
| LRF0818C | 1535 nm | 0.4 mrad | 0.4 m | 26 mm | 300 µJ | 10 Hz |
| LRF0609C | 1535 nm | 0.5 mrad | 0.5 m | 26 mm | 200 µJ | 10 Hz |
| LRF0610C | 1535 nm | 0.5 mrad | 0.5 m | 10 mm | 200 µJ | 10 Hz |
| LRF0405C | 1535 nm | 0.6 mrad | 0.6 m | 8 mm | 200 µJ | 10 Hz |
| LRF0305C | 1535 nm | 0.6 mrad | 0.6 m | — | 100 µJ | 10 Hz |
| LRF0306C | 1535 nm | 0.6 mrad | 0.6 m | — | 100 µJ | 3 Hz |
| LRF0310C | 1535 nm | 0.6 mrad | 0.6 m | 8 mm | 100 µJ | 10 Hz |
| LRF0105C | 1535 nm | 1 mrad | 1.0 m | 8 mm | 100 µJ | 10 Hz |
| LRF1831C | 1535 nm | 1.3 mrad | 1.3 m | 60 mm | 350 µJ | 10 Hz |
| ER10000 | 1535 nm | 4 mrad | 4.0 m | — | 10 µJ | 5 Hz |
| ER2000 | 1535 nm | 4 mrad | 4.0 m | — | 2 µJ | 10 Hz |
| ER4000 | 1535 nm | 4 mrad | 4.0 m | — | 4 µJ | 5 Hz |
| ER8000 | 1535 nm | 4 mrad | 4.0 m | — | 8 µJ | 5 Hz |
| LR1200E2 | 905 nm | 4 mrad | 4.0 m | 9.2 mm | — | 10 Hz |
| LR1200E4 | 905 nm | 4 mrad | 4.0 m | 9.2 mm | — | 10 Hz |
| SPD1200N0 | 905 nm | 4.5 mrad | 4.5 m | 6.5 mm | — | 15 Hz |
| SPD1200N2 | 905 nm | 4.5 mrad | 4.5 m | 6.5 mm | — | 15 Hz |
| SPD1200N4 | 905 nm | 4.5 mrad | 4.5 m | 6.5 mm | — | 15 Hz |
| LR1000D23 | 905 nm | 6 mrad | 6.0 m | 20 mm | — | 12 Hz |
| LR1200D23 | 905 nm | 6 mrad | 6.0 m | 20 mm | — | 10 Hz |
| LR1500D23 | 905 nm | 6 mrad | 6.0 m | 20 mm | — | 10 Hz |
| LR1500E2 | 905 nm | 6 mrad | 6.0 m | 9.2 mm | — | 10 Hz |
| LR1500E4 | 905 nm | 6 mrad | 6.0 m | 9.2 mm | — | 10 Hz |
| LR2000E2 | 905 nm | 6 mrad | 6.0 m | 9.2 mm | — | 10 Hz |
| LR2000E4 | 905 nm | 6 mrad | 6.0 m | 9.2 mm | — | 10 Hz |
| SPD1200N3 | 905 nm | 6 mrad | 6.0 m | — | — | 15 Hz |
| SPD1200S2 | 905 nm | 6 mrad | 6.0 m | 9 mm | — | 15 Hz |
| SPD1200Z2 | 905 nm | 6 mrad | 6.0 m | — | — | 20 Hz |
| SPD1200ZG | 905 nm | 6 mrad | 6.0 m | 6.5 mm | — | 10 Hz |
| ER300 | 1535 nm | 7 mrad | 7.0 m | — | 300 µJ | 10 Hz |
| ER400 | 1535 nm | 7 mrad | 7.0 m | — | 400 µJ | 10 Hz |
| ER500 | 1535 nm | 7 mrad | 7.0 m | — | 500 µJ | 10 Hz |
| ER800 | 1535 nm | 7 mrad | 7.0 m | — | 800 µJ | 10 Hz |
| ER900 | 1535 nm | 7 mrad | 7.0 m | — | 900 µJ | 5 Hz |
| ER100 | 1.54 µm | 8 mrad | 8.0 m | — | 100 µJ | 10 Hz |
| ER200 | 1535 nm | 8 mrad | 8.0 m | — | 200 µJ | 10 Hz |
| LR1000E2 | 905 nm | 9 mrad | 9.0 m | 9.2 mm | — | 10 Hz |
| LR1000E4 | 905 nm | 9 mrad | 9.0 m | 9.2 mm | — | 10 Hz |
| MINI-100 | 1535 nm | 10 mrad | 10.0 m | — | 100 µJ | 10 Hz |
| LRF3000A1 | 905 nm | 10 mrad | 10.0 m | — | — | 10 Hz |
| LRF1200A1 | 905 nm | — | — | 6.6 mm | — | 3 Hz |
What the numbers mean together
- Divergence sets the spot: 0.3 mrad is 0.3 m at 1 km and 6 m at 20 km. A target smaller than the spot behaves as a point target — return falls with the fourth power of distance.
- Receiver aperture is the second-largest lever after pulse energy: received power scales with area, so doubling the diameter quadruples the collected return. That is why the long-range modules carry 60 mm receivers and the 905 nm sensors carry 6.5 mm.
- Pulse energy is limited by eye safety at each wavelength: a 905 nm design cannot carry the energy a 1535 nm design can, which is the entire reason two wavelength families exist.
- Update rate trades against energy: the 1535 nm sources run 0.5–10 Hz because a rod is being pumped, while silicon-detector modules reach kilohertz.
Where a figure is not published, this table shows a dash. Do not read a dash as
zero — read it as "ask the manufacturer before you assume".
Working out the photon budget?
Send the target size, the reflectance and the distance you need to cover.
Email tommy@erdimail.com
Divergence and aperture explained
Transcribed 2026-10-23; spot diameter = divergence × distance (initial beam diameter ignored). Each row links to its model page. Dataset: CSV.