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Spectra CT Luminance Standard

Adjustable CCT Uniform Light Source Luminance Standard

The Labsphere Spectra CT luminance standard is a uniform light source that combines separate warm white and cool white LEDs that provides for continuous adjustment of correlated colour temperature (CCT) between 2800 and 7500 Kelvin. The Spectra CT is available with 20, 30 and 50cm sphere diameters and with corresponding exit ports of 5, 10 and 20cm. Depending on model, luminance is continuously adjustable over a wide range from 0-50,000 cd/m2. The Spectra CT can be used to calibrate a wide range of photometric test equipment and imaging devices but is particularly well suited for testing imaging colorimeters that are used to characterise and calibrate electronic display devices.

The Spectra CT-1000 uniform light source serves as a standard of luminance with which you can adjust both the luminance and also the correlated colour temperature (CCT), the shade of white light. By combining separate warm white and cool white LEDs, the CCT can be continuously adjusted between 2800 and 7500 Kelvin. This allows for the flat field correction and the calibration of camera systems, reducing colorimetric errors due to the matching of the calibration CCT to the target illuminant that the camera will be used to measure.

The CT-1000 is available in three sphere sizes of 20, 30 and 50cm sphere diameters and with corresponding exit ports of 5, 10 and 20cm. The luminance of the CT-1000-S (20cm sphere) can be adjusted from 1-50,000 cd/m2, while that for the CT-1000-M (30cm sphere) spans the range 0.5-25,000 cd/m2. The luminance range for the CT-1000-L (50cm sphere) is 0.1-5,000 cd/m2. Luminance adjustment is accomplished by means of programmable LED drive currents.

An integrated luminance photometer reports the real-time output brightness of the sphere. The CT-1000 is controlled via a USB interface from a user-provided PC running Labsphere’s LSS-PT software. The operator can set both a target luminance and CCT using the software.

Spectra CT Luminance Standard

Uniform Light Source Theory

An internally illuminated integrating sphere simplifies what would otherwise be complex procedures in the calibration and distortion correction of cameras and image sensors. Generating a field of uniform irradiance or radiance is not easy – unless you use an internally illuminated integrating sphere. Any light entering a sphere reflects with equal radiance in all directions from the diffusely reflecting (Lambertian) sphere wall coating. The high reflectance coating (typically 96-99%) ensures a high number of reflections, resulting in a near-perfectly uniform radiance at all points on the sphere wall. The open exit port on an internally illuminated integrating sphere is the “uniform source”. The sphere can be illuminated by lamps or LEDs placed inside the sphere or held outside at a sphere port.

A uniform light source integrating sphere functions both as a source of uniform radiance and irradiance. A camera whose lens is focussed onto the plane of the exit port of the sphere collects defocussed light from the sphere wall opposite. The irradiance is uniform at all points on the sphere wall, and the wall reflects light with constant radiance at all angles. Therefore, the camera sees a field of uniform radiance or luminance. Without imaging optics, the integrating sphere would deliver a field of uniform irradiance directly onto an image sensor. An image sensor placed directly in the plane of the exit port of the sphere receives uniform (but diffuse) irradiance. Note that the irradiance uniformity decreases in the near-field, but recovers in the far-field.

The Need for Uniform Radiance/Irradiance with Image Sensors & Cameras

Focal plane array (FPA) image sensors (PDA, CMOS, CCD etc) suffer from pixel-to-pixel differences in responsivity (photo response non-uniformity, PRNU) as well as photon (shot) noise, dark (thermal) noise, read noise and non-linearity. By placing the sensor at the exit port of a uniform light source, we uniformly illuminate each pixel on the array and can perform pixel gain and offset normalisation. An imaging system (reflective or refractive) introduces additional distortions with angle: vignetting and cos4 intensity drop-off. An integrating sphere uniform light source provides spatially and angularly uniform radiance and allows the camera (sensor with lens) to be flat field corrected.

 

Spectra CT-1000

Light Source

Warm white & cool white LEDs

Luminance Range*

CT-1000-S: 1-50,000 cd/m2

CT-1000-M: 0.5-25,000 cd/m2

CT-1000-L: 0.1-5,000 cd/m2

Colour Temperature (CCT)

Adjustable from 2800 to 7500K

Integrating Sphere

CT-1000-S: 20cm diameter Spectraflect

CT-1000-M: 30cm diameter Spectraflect

CT-1000-L: 50cm diameter Spectraflect

Exit Port Diameter

CT-1000-S: 5cm diameter

CT-1000-M: 10cm diameter

CT-1000-L: 20cm diameter

Luminance Adjustment

Programmable LED DC drive current, 5 x 104 steps

Luminance Spatial Uniformity**

99% (COV)

Interface

USB

Software

Labsphere LSS-PT (Windows 10)

Calibrations

Luminance (cd/m2)

Correlated colour temperature (CCT)

Spectral radiance at peak luminance (W/sr.m2.nm, 350-2400nm)

Spatial uniformity

Power

TBA

Dimensions/Weight

CT-1000-S: 35 x 38 x 28cm, 10kg

CT-1000-M: 51 x 48.5 x 33cm, 15kg

CT-1000-L: 72.5 x 71.5 x 57cm, 35kg

* Luminance range will vary with CCT set point
** Luminance uniformity calculated per NIST COV method

Focal plane array (FPA) image sensors (PDA, CMOS, CCD etc) suffer from pixel-to-pixel differences in responsivity (photo response non-uniformity, PRNU) as well as photon (shot) noise, dark (thermal) noise, read noise and non-linearity. By placing the sensor at the exit port of a uniform light source, we uniformly illuminate each pixel on the array and can perform pixel gain and offset normalisation.

An imaging system (reflective or refractive) introduces additional distortions with angle: vignetting and cos4 intensity drop-off. An integrating sphere uniform light source provides spatially and angularly uniform radiance and allows the camera (sensor with lens) to be flat field corrected.

The Spectra CT not only provides for a uniform luminance field to perform flat field correction and linearity correction of camera systems, but by virtue of the tuneable colour temperature, it also improves the accuracy of the camera by matching the colour point used in the calibration to the CCT that the camera will be used to image in practice. Typical applications for the CT-1000 include the calibration, flat field correction, linearity calibration, and dark correction of display panel inspection cameras, in-vehicle cameras, cameras and ambient light sensors in consumer electronics and luminance meter and colorimeter response correction.

Uniform Light Source Camera Correction

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