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COLOR TEMPERATURE<br />

KELVIN COLOR TEMPERATURE (K)<br />

This is the scientific temperature scale used to designate the spectral output <strong>of</strong> a radiant element such as a lamp<br />

filament sufficiently heated so that it emits visible light. Such heated elements will then produce a continuous visible<br />

spectrum, with some output at all wavelengths. Examples include incandescent and tungsten sources, as well as<br />

natural daylight.<br />

Simply put, a lower kelvin temperature indicates a relatively higher amber output, while a higher kelvin temperature<br />

corresponds to a relatively higher blue output.<br />

CORRELATED COLOR TEMPERATURE (CCT)<br />

This is a term <strong>of</strong>ten applied to arc sources that do not employ a heated filament and thus do not produce a continuous<br />

visible spectrum. Examples include fluorescent lamps and industrial discharge lamps.<br />

For color correction purposes in film and electronic imaging, the manufacturer’s suggested Correlated Color<br />

Temperature <strong>of</strong> these sources should not be employed, unless the accompanying Color Rendering Index (CRI)<br />

exceeds a value <strong>of</strong> 90 (e.g. HMI or Electronic Strobe).<br />

COLOR TEMPERATURE AND MIRED SHIFT VALUE<br />

The kelvin color temperature scale is not the best method for predicting the effect <strong>of</strong> color correction filters. This<br />

is because the resulting kelvin temperature will vary, depending upon the kelvin temperature <strong>of</strong> the original source.<br />

For example, Half Blue will increase kelvin 900 degrees for a 3200K source, yet only 600 degrees for a 2600K<br />

source, and 1500 degrees for a 4000K source.<br />

Mired Shift Value is a constant value. It provides an accurate method for predicting the effect <strong>of</strong> a color correction<br />

filter regardless <strong>of</strong> the kelvin temperature <strong>of</strong> the original source. It also allows for predictable results when combining<br />

filters, since the mired shift values are additive or subtractive.<br />

Note: This process <strong>of</strong> calculating mired shift value is vastly simplified through the use <strong>of</strong> the Rosco <strong>Filter</strong><br />

Nomograph (pg. 8). In addition, Rosco <strong>of</strong>fers an easy to use, electronic calculator that determines either the<br />

required filter or the resulting kelvin from selected filters. Both the <strong>Filter</strong> Nomograph and the Electronic Calculator<br />

are available for free download at www.rosco.com.<br />

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