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IR Illumination Design for Depth Sensing

The physics and engineering of infrared illumination systems for ToF and structured light depth cameras.

Evyatar Bluzer
2 min read

Depth sensors need light to see. Unlike passive cameras that use ambient light, active depth sensors emit their own illumination - typically in the near-infrared (NIR) spectrum around 850nm or 940nm.

Why NIR?

Invisible to users: 850nm+ is outside human visual range Efficient sources: VCSELs and LEDs are mature at these wavelengths Sensor sensitivity: Silicon sensors still respond well (though sensitivity drops above 900nm) Sunlight filtering: Narrow bandpass filters can reject most solar spectrum

Illumination Architectures

Flood Illumination (ToF)

Cover the entire field of view with uniform IR light. Simple conceptually, but challenges include:

  • Uniformity: Edges of FOV receive less light (cosine falloff + lens vignetting)
  • Power density: More range requires more power, but eye safety limits peak intensity
  • Efficiency: Much light falls on areas we don't need (sky, distant objects)

Patterned Illumination (Structured Light)

Project a known pattern (dots, lines, speckle) and use deformation for triangulation.

  • Diffractive Optical Elements (DOE): Split single beam into pattern - very power efficient
  • Pattern design: Must be unique enough for unambiguous matching
  • Density trade-off: More points = more resolution but harder matching

Spot Illumination (Scanning)

Single beam scanned across the scene (like LiDAR).

  • Power efficient: All energy concentrated in measurement point
  • Slow: Mechanical scanning limits frame rate
  • Eye safety: Easier to manage with low duty cycle per point

Design Constraints

For our headset:

  • Eye safety: IEC 62471 Class 1 limits power density at the eye
  • Power budget: under 200mW for illumination
  • Range: 0.3m to 5m indoor, 0.3m to 3m outdoor
  • Ambient rejection: Must work in 10,000 lux sunlight

The math is harsh. Sunlight at 940nm contributes ~0.2 mW/cm²/nm. Our narrow filter (10nm bandwidth) still passes 2 mW/cm². We need to exceed this with our illumination at 5m range while staying within power and safety budgets.

Multi-Frequency Approaches

One promising direction: modulate illumination at frequencies where ambient light doesn't contribute. Time-domain or frequency-domain filtering can reject DC (sunlight) while preserving our modulated signal.

Next month: diving deeper into the optics design.

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