UV Photodiode

Generates a photocurrent proportional to UV irradiance in a defined sub-band (200–280 nm UV-C, 280–315 nm UV-B, or 315–400 nm UV-A), output through a transimpedance amplifier as a calibrated UV index or W/m² value.

A wide-bandgap semiconductor PN junction (SiC's 3.26 eV or GaN's 3.4 eV) absorbs photons whose energy exceeds the bandgap, generating electron-hole pairs that the bias field separates into photocurrent. Bandgap-tuning makes the sensor blind to wavelengths longer than its cutoff (e.g., a 280 nm SiC sensor is solar-blind). On-chip optical filters narrow the response to a specific UV sub-band; a TIA converts photocurrent to voltage.

In plain terms

Like a smoke detector that sees only the colour of fire — invisible to room lights and sunlight, but lights up the moment a UV-emitting flame appears.

Why designers use it

Best for

Key specifications

When not to use it

Common mistakes

Where you will find it

A short history

UV photodiodes detect radiation in the 200–400 nm ultraviolet band, below the range of conventional silicon photodiodes, which are blind to wavelengths below ~350 nm without special coatings. Hamamatsu Photonics, founded in Japan in 1953, became a leading developer of UV-sensitive photodetectors using silicon with UV-enhancing surface treatments, and later gallium nitride and silicon carbide (SiC) junctions that have bandgaps suited to UV detection with suppressed visible-light response ("solar-blind" behaviour). UV photodiodes are essential in flame detectors for gas turbines and boilers (UV emission of a hydrocarbon flame), UV-index sensors for consumer wearables, ozone monitoring, and UV-curing process control in printing and semiconductor lithography. The development of GaN-based UV photodiodes in the 1990s enabled compact, solid-state flame sensors that replaced vacuum-tube UV tubes.

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