Integrating Sphere

A hollow white ball that turns any light source — directional or messy — into a perfectly uniform glow you can measure.

An integrating sphere is a hollow cavity (25 mm to 2 m diameter) whose interior is coated with a diffuse Lambertian reflector — barium sulfate (~97 % reflectance) or sintered PTFE 'Spectralon' (~99 %). Light entering through one port reflects diffusely tens of times, becoming spatially uniform across the sphere wall. A small detector port reads radiance proportional to total input flux, regardless of source directionality, polarization, or beam shape. Used to measure: total LED/lamp luminous flux (lumens), laser power independent of mode structure, sample diffuse reflectance/transmittance, and as a uniform calibration source for cameras.

A Lambertian surface reflects with intensity I(θ) ∝ cos θ — equal radiance from any viewing angle. After many reflections, the photon distribution converges to spatial uniformity. The 'sphere multiplier' M = ρ / [1 − ρ(1 − f)], where ρ is wall reflectance and f is the port-area fraction, quantifies how much brighter the wall radiance is than a single-bounce expectation. For ρ = 0.97 and f = 0.02, M ≈ 32 — meaning a typical photon bounces ~32 times before being detected. Sphere wall radiance L = ρ Φ_i / [4π r² (1 − ρ(1−f))]. A baffle is placed between the source illumination spot and the detector port so the detector sees only multiply-reflected (integrated) light, not the first reflection. Calibration uses a NIST-traceable reference lamp; relative measurements (substituting a known reference into the same sphere) avoid absolute calibration drift. The auxiliary-lamp method corrects for self-absorption when the source itself absorbs sphere light.

In plain terms

Imagine a perfectly white, perfectly round room. Any flashlight you point in any direction bounces around the walls so many times that every corner glows the same. You can put a light meter anywhere and get the same reading — and the reading tells you the total amount of light, no matter which way the flashlight was pointing. That's an integrating sphere.

Also called: Ulbricht sphere, photometric sphere, Lambertian cavity.

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A short history

W. E. Sumpner published the theoretical principle of the integrating sphere in 1892. Richard Ulbricht published its practical design in Germany in 1900 — hence 'Ulbricht sphere.' The technique became standard for incandescent and fluorescent lamp photometry through the 20th century. With the rise of LEDs, integrating spheres became central to solid-state-lighting metrology; CIE Publication 84 (1989) and CIE S 017:2020 codify the practice. Spectralon (Labsphere) introduced sintered-PTFE coatings in the 1980s, raising the achievable reflectance to ~99 %.

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