Posts Tagged ‘color theory’

Color Rendering Index

Monday, July 6th, 2009

Equally important as the correlated color temperature for fluorescent lamps, the color rendering index (CRI) is used to determine how things are going to look under fluorescent lighting. The CRI is a made-up scale ranging from 0 to 100, where 100 is the expected color rendition of incandescent/halogen sources

The colors of objects that you see are actually those colors being reflected back at you. If you start with white light shining on “red” object, the blue and green parts of the white light are absorbed by the object and the red is reflected back for you to see. If instead of a “white” light that has a good balance of red, blue, and green, you have a “white” light that is weak in the red part, the blue and green still get absorbed by the object, but there is less red to be reflected back at your eye. The same object is going to look less “red” under the second “white” light.

Since an incandescent source is like a black-body radiator, the color spectrum of of the light generated by the filament has a decent mix of all the visible colors. However, since the colors present in the “white” light of a fluorescent is made up by phosphors which each do just a part, there can be a poor mix of colors in the light. The better the phosphors do at creating that mix of colors the better the CRI rating.

The more important color is, the higher the CRI of your lamp should be. Manufacturers will make similar lamps (in terms of size, power, etc.) with different CRI ratings since the lower CRI lamps can be made more cheaply. People will either select the lower CRI lamps because color doesn’t matter as much as cost or because they don’t know that there is a difference. For example, for linear tube fluorescents, like you find in offices, the cheaper lamps will have CRI ratings in the low to mid 70s and the higher quality lamps will have CRI rating in the low to mid 80s.

For your home or office I recommend getting the lamp with the highest CRI you can find. For standard fluorescents I only specify lamps with a minium CRI of 85. For compact fluorescents I have to drop my minimum to a CRI of 82, since higher CRI rated lamps aren’t readily available.

Note that both the CRI and the CCT of a fluorescent lamp will be printed on the lamp itself, so if you need to find out what something is you can just look at it. For a linear tube style, the information will be printed on the glass at one of the ends. For a compact fluorescent lamp the information will be printed on the base. Most of the time the information is just printed as “82 CRI” and “3500K.” Sometimes only the manufacturer’s coding will be printed, but typically it will show the CRI by either a “7″ or “8″ somewhere in the lamp code (for low to mid 70’s or low to mid 80’s as appropriate) and the CCT as the first two digits of the CCT (such as 27 for 2700K or 35 for 3500K).

To see an example of what happens when you use a lamp with a low CRI rating most people can probably just find a nearby streetlight. Many streetlights are still high-pressure sodium because HPS lamps are very energy efficient. However, they also have a CRI around 22 and a CCT of around 1800K. That’s why the “orange glow” of a streetlight makes everything look orange or gray.

If you have streetlight around you that look more “white” than orange they are either very old mercury lamps (which are now banned from new installation but utility companies who stockpiled them can use up their inventory until they replace the fixture) or metal halide lamps. They probably have a CCT of around 4000K and a CRI ranging from about 50 (mercury vapor) to 65 to 75 (metal halide). There are also new ceramic metal halide lamps that can have a CRI as high as the low to mid 90’s.

Using streetlights doesn’t provide a perfect example since the darkness of night also affects how we perceive colors, but it’s a good shorthand.

Color Temperature Basics: What is It?

Wednesday, July 1st, 2009

Color temperature refers to a “black-body radiator.” This is a theoretical object (as in, it doesn’t really exist but we pretend it does because we find that useful) that will absorb all electromagnetic radiation cast upon it; it will reflect or transfer none. Visible light is a small portion of electromagnetic radiation, which you can think of as the stuff coming from the sun that provides light and heat.

When a black body radiator is heated it begins to glow. There’s a cool java applet on the Olympus Microscopy Resource Center website that demonstrates this idea with a picture of a horseshoe. At the lower range it begins by glowing red. Then as it gets hotter it goes through yellow and white phases, eventually shifting into the very bright blue-white range. At any particular color, we refer to the temperature of the blackbody as the “color temperature.” (A note on that java tutorial, the temperature indicated on the scale refers to the tips of the horseshoe. The other colors move down the horseshoe to show that the tips are being heated and the bottom is cooler than the tip. The temperature does not relate to all the colors shown in the image.) The temperature is on the Kelvin scale, which is the same as celsius plus 273. That is, -273˚C is 0 K, 0˚C is 273 K, and 100˚C is 373 K.

For lighting, it is easier to refer to the temperature generating a color than trying to describe the color itself, which changes slowly and is not really part of our language of color. If you are looking at that java applet from Olympus, try to describe the difference between the color of the horseshoe tips at 2700K, 3000K, and 3200K. You’ll quickly realize why referring to a color temperature is easier.

A bit of confusing terminology, however, is that we refer to red the red side as “warm” and the blue side as “cool.” This is based on our traditional color associations of red and blue. It can be confusing because the bluer tint comes as you increase the temperature. Hence, you may hear people refer to “raising” the color temperature to “cool” the light source.

The filament of a regular incandescent lamp is not a true black-body, but it does go through the same color process as it is heated. That’s why when you put a regular lightbulb on a dimmer it shifts toward the red as you dim it down: it’s the horseshoe in reverse. Therefore, if you’re looking at incandescent lightbulbs color temperature isn’t a very useful metric. Regular and halogen lamps at full power usually end up around 2700K to 3050K, and that can be changed by adjusting the voltage. The real purpose of discussing color temperature is for fluorescent lamps, which I’ll get to tomorrow.

Color Temperature Basics: Why Should You Care?

Tuesday, June 30th, 2009

I mentioned during the introduction to fluorescents that I would have follow-up posts about color temperature and CRI (color rendering index). I’m going to kick this off with color temperature and an explanation of why anyone would care about it.

relative-color-2One of the biggest problems with artificial lighting is that our eye and brain determine a lot of color information by comparison instead of some sort of mental color wheel. I’ve stuck an image file into this post to provide an example. The image to the right is made up of exactly 3 colors, but the purple color appears to be either a lighter or darker purple depending upon whether the adjacent color is the blue or the pinkish color. Also, the purple bar that runs all across the middle seems to change color from one side to the other.

The issue for artificial lighting is that as we look around us, our eye spots the brightest source of light and our brain “sets” that as white light. We are mentally doing the opposite of the what my sample image shows: instead of using relativity of colors to “see” either bright or darker versions of purple when the purple is actually the same, we are using relativity of colors to see different versions of “white” and then perceiving that as always the same “white.”

For the common user, a lightbulb (unless a specialty colored lamp) is going to be perceived as white. For the professional, we know that different sources are giving us different whites and we need a way to document the differences. We do that by specifying the “color temperature” of the source.

For the next post, I’ll explain what color temperature actually is and how we come up with the numbers.