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Photometry is related to Radiometry, and the lumen to the watt, by a simple mathematical model of the spectral sensitivity of the human visual system. This model is represented by the spectral luminous efficiency function, V(λ). By definition, the luminous flux of a source, ΦL, is related to its spectral radiant flux, Φ(λ), by the application of a weighted integral, as indicated in the equation below. Note that - for historical reasons - the unitless V(λ) function is normalized at a peak value of 683 (lm/W):
When spectroradiometric data is available, photometric data can be derived by weighted integration, as indicated above. An alternative approach involves the construction of a sensor with a relative spectral response which closely approximates the V(λ) function. Such a device is known as a photometric or photopic sensor.
UDT Instruments offers a line of photometric components that support the configuration of a wide range of system solutions. Our applications engineers are ready to work with you to recommend a solution that fits your exact requirements. |
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UDT Instruments 8581 Aero Drive, San Diego, CA 92123 USA Phone: +1-858-279-8035 Toll Free: 1-877-532-5800 |