Photocurrent Calculator

Model photodiode response using quantum efficiency and power. Include gain, area, and dark current effects. Get clear current outputs for lab and design work.

Optical input
Choose direct power or compute power from irradiance and detector area.
Use average power at the detector plane.
Uniform illumination assumption improves accuracy.
Use the photosensitive area, not package size.
Detector responsivity
Use quantum efficiency and wavelength, or enter responsivity directly.
In nanometers; match your source spectrum peak.
Percent of photons producing carriers.
A/W at your operating wavelength.
Electrical options
Gain models amplifier or internal multiplication.
Use 1 for no amplification.
In nA; depends strongly on temperature.
Saved into exported files.
Reset

Formula used

How to use this calculator

  1. Select an optical input method: direct power or irradiance × area.
  2. Enter power, or provide irradiance and active area with units.
  3. Select a responsivity method: quantum efficiency or direct responsivity.
  4. Enter wavelength and quantum efficiency, or enter responsivity in A/W.
  5. Set gain and dark current to match your measurement chain.
  6. Press Calculate to view results above the form.
  7. Use CSV or PDF buttons to export the computed report.

Example data table

Case Method Optical input Wavelength QE Gain Dark current Expected photocurrent
A Direct power 2.0 mW 850 nm 70% 1 5 nA ≈ 0.77 mA
B Irradiance × area 1.2 mW/cm², 9 mm² 940 nm 55% 10 20 nA ≈ 0.29 mA
C Direct responsivity 250 µW 5 2 nA R=0.45 A/W → ≈ 0.56 mA

Examples are illustrative and depend on spectral response and bias conditions.

Photocurrent guide

1. What photocurrent represents

Photocurrent is the light-generated current from a photosensor. For a linear photodiode region, it scales with optical power and responsivity. If your circuit includes transimpedance gain or internal multiplication, the measured current can be higher than the raw diode current.

2. Optical power versus irradiance

Many datasheets quote responsivity in A/W, which expects total optical power at the active area. When only irradiance is known, power is computed by P = E × A. The calculator supports W/m² and mW/cm², plus area units m², cm², and mm².

3. Responsivity from quantum efficiency

When quantum efficiency is available, responsivity is estimated using R = η q λ /(h c). As a reference, η=70% at 850 nm yields about 0.48 A/W. At 940 nm, η=55% gives roughly 0.40 A/W. These values are typical for silicon near its sensitivity peak.

4. Wavelength and spectral mismatch

Real sources are not monochromatic. LEDs can have 20–50 nm spectral width, while lasers are much narrower. If the spectrum shifts, responsivity can change significantly near cutoffs. For silicon, responsivity drops approaching ~1100 nm. Use the wavelength that best matches your dominant optical energy.

5. Dark current and offset handling

Dark current adds an offset, modeled here as Itotal = Iphoto + Idark. Dark current can be a few nA for small diodes at room temperature, but it can rise by orders of magnitude with temperature and reverse bias. Enter your measured dark current for best results.

6. Gain and measurement chains

The gain field can represent amplifier scaling or multiplication devices. For example, a gain of 10 applied to a 30 µA photocurrent produces a 300 µA output. When using a transimpedance stage, convert voltage output to current-equivalent gain if you want a consistent current budget.

7. Practical accuracy checks

Confirm linearity by testing two power levels. If power doubles, the photocurrent should double within measurement error. Watch for saturation from limited bias, amplifier headroom, or high irradiance. Also verify units: 1 mW/cm² equals 10 W/m², a common source of mistakes.

8. Typical use cases and ranges

Photocurrents can span pA to mA. Low-light sensing and spectroscopy often operate in pA–nA with careful shielding. Proximity sensing and optical communication receivers commonly sit in µA–mA depending on optics and responsivity. Use the export tools to document inputs and results for lab reports.

FAQs

1) Should I use quantum efficiency or responsivity?

If your datasheet provides responsivity at the operating wavelength, enter it directly. Use quantum efficiency when responsivity is missing or you want a wavelength-based estimate from η and λ.

2) Why does wavelength change the result?

Responsivity depends on how efficiently photons create carriers. The photon energy and sensor material response vary with wavelength, so the same optical power can produce different currents at different wavelengths.

3) What area should I enter for irradiance mode?

Enter the active photosensitive area that is illuminated. If the beam is smaller than the diode, use the beam spot area. If the beam is larger, use the diode’s active area.

4) How do I include losses from windows or filters?

Apply the transmission factor to power. For example, 80% transmission means P = 0.8 × Psource. You can also reduce irradiance by the same factor before calculating.

5) Why is my measured current higher than predicted?

Possible reasons include internal gain, amplifier scaling, stray light, or responsivity higher than assumed. Check whether you are measuring output current after gain and confirm your power measurement plane matches the detector plane.

6) What does dark current mean in practice?

Dark current is current that flows without light due to leakage and thermal generation. It contributes offset and noise. Measure it under the same bias and temperature used for your light measurement.

7) Can I use this for pulsed sources?

Yes, if you use average optical power for average photocurrent. For peak photocurrent, use peak power and ensure the detector and electronics bandwidth support the pulse width without distortion.

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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.