Measure light output with flexible modes and units. Follow simple steps for reliable optical calculations. Export your results to files in seconds easily now.
| Scenario | Inputs | Method | Radiant Power (W) |
|---|---|---|---|
| Illuminated sensor patch | E = 320 W/m², A = 0.015 m² | Irradiance × Area | 4.8 |
| Directional emitter | I = 2.5 W/sr, Ω = 0.8 sr | Intensity × Solid Angle | 2.0 |
| Pulsed optical burst | E = 18 J, t = 0.25 s | Energy ÷ Time | 72 |
The calculator converts inputs into SI units internally, then returns the solved quantity. Use consistent geometry for area and solid angle to avoid systematic errors.
Radiant power (Φ) is the total optical energy emitted, transferred, or received per second. It is measured in watts, and it is a starting point for comparing sources such as LEDs, lamps, and lasers, regardless of beam shape.
When you know the illuminated area, irradiance (E) links directly to power through Φ = E × A. This supports detector work, solar testing, and exposure checks where the footprint is measurable and the average level is meaningful.
For directional emitters, radiant intensity (I) describes power per unit solid angle (W/sr). The relationship Φ = I × Ω estimates total output if the emission cone is known. Narrow beams require careful geometry because small Ω errors can shift results.
Radiant exitance (M) is emitted power per unit area from a surface. Using Φ = M × A is common in thermal radiation and hot-surface assessments. It helps when the source is a panel, filament, or heated plate with a defined emitting region.
For pulsed systems, average radiant power follows Φ = Er / t. Energy in joules may come from a pulse-energy meter, while time can be pulse duration or a measurement window. This mode also supports integrating sensors that report total energy.
This calculator converts inputs to SI internally, then performs the selected solve step. Conversions like mW/cm2 to W/m2 or msr to sr reduce manual mistakes. Always confirm that the area and angular definitions match your setup.
Radiant-power estimates are only as good as the measurements behind them. Nonuniform beams, misaligned apertures, and partial collection can bias results. When possible, repeat measurements, record geometry, and note instrument calibration and wavelength limits.
A practical workflow is to measure a footprint, compute power from irradiance, and compare against a rating. For sources with known optics, compute power from intensity and solid angle. For pulsed sources, use energy and time to validate average output.
Radiant power is total optical output in watts. Radiant intensity is power per solid angle in W/sr, describing how concentrated the emission is in a direction.
Use it when you know the average irradiance over a defined area, such as a beam footprint on a target. It works best when the field is close to uniform.
For a circular cone with half-angle θ, solid angle is Ω = 2π(1 − cosθ). Ensure θ matches the emission or collection geometry used in your setup.
Yes. If you know radiant exitance M (W/m²) and emitting area A, then Φ = M × A. This is useful for plates, panels, and other extended emitters.
It gives average radiant power over the chosen time interval. For pulses, energy may be per pulse, and time may be pulse duration or a measurement window.
If the physical inputs are identical, results should match. Differences usually indicate an incorrect unit choice, a scale mismatch, or inconsistent area and footprint values.
It can support early estimates, but safety decisions need standards-based limits, spectral weighting, and verified procedures. Use calibrated instruments and consult relevant guidelines for final evaluations.
Important Note: All the Calculators listed in this site are for educational purpose only and we do not guarentee the accuracy of results. Please do consult with other sources as well.