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Color Temperature

The concept of color temperature is based on the relationship between the temperature and radiation emitted by a theoretical standardized material termed a black body radiator cooled down to a state in which all molecular motion has ceased. Hypothetically, at cessation of all molecular motion, the temperature is described being at absolute zero or 0 Kelvin, which is equal to -273 degrees Centigrade.

Imagine now that the black body radiator is heated to the temperature of freezing water, equal to 273 Kelvin, 0 degrees Centigrade, or 32 degrees Fahrenheit. The black body is then further heated to the temperature of boiling water: 373 Kelvin, 100 degrees Centigrade, or 212 degrees Fahrenheit. If the black body continues to be heated, it will begin to glow and give off its own light. When the temperature reaches 3200 Kelvin, the radiator will be emitting light with a visible spectrum equal to the color temperature of light produced by a tungsten filament, typical of those found in microscope lamps.

The absolute temperature of a black body radiator is always expressed in Kelvin, which is equivalent (the degree increments are identical) to degrees Centigrade (C) plus 273 degrees. For example, 1000 K equals 727 C. Therefore, we can define the color temperature of a light source as the value of the absolute temperature of a black body radiator when the radiator chromaticity matches that of the light source. In the case of fluorescent lamps and other sources that can only approximate the chromaticity of a black body, the corrected term correlated color temperature is applied through a calculated chromaticity.

Although this black body radiator does not actually exist, many metals behave in a similar manner, so we can employ a black metal horseshoe (Figure 1) as an example for this discussion. In Figure 1, the horseshoe is first heated to a temperature of about 900 K (Figure 1(a)), where it begins to glow a dull red. As the temperature is increased to between 1500 K and 2000 K, the horseshoe (Figure 1(b)) turns a yellowish to brighter red color. Increasing the temperature still further to just over 3000 K produces a yellow-to-white color transition (the color temperature of a tungsten filament, Figure 1(c)), and at 5000 K and above (the color temperature of daylight, Figure 1(d)), a bluish-white color appears. This concept can be further investigated in our interactive Java-powered color temperature tutorial linked below.

Interactive Java Tutorial
Color Temperature
Explore how color temperature is affected by changes in the temperature of a black body radiator. 

The concept of color temperature is very important in photography, where film emulsions must be balanced to accurately render color using different light sources. This is especially true in photography through the microscope. Films intended to be used outside in ordinary daylight, or indoors with fluorescent or flash lighting, are balanced during manufacture for a color temperature of 5500 K. Alternatively, films designed for use indoors with tungsten light bulbs (or in the microscope) are balanced for a color temperature of 3200 K to 3400 K. The 5500 K average value of the daylight color spectrum varies during different parts of the day and is also season-dependent (see Table 1). In the early morning and late evening, the color temperature will fall to 5000 K and below, causing color shifts in the emulsion that result in warmer (redder) color renditions.

There are two important points to consider when examining color temperature phenomena. The color temperature value of a light source refers only to the visual appearance of the source, but does not necessarily describe the effect this source will have on photographs or photomicrographs. Also, color temperature does not take into consideration the spectral distribution of a visible light source. In cases where a light source, such as a fluorescent lamp, laser, or gas lamp, does not have a spectral distribution similar to that of a black body radiator, its color temperature alone is not a reliable means of selecting suitable filters for color balance corrections. Therefore, although two different light sources may be described as having the same color temperature, exposed photographic emulsions may respond differently to the sources. When using fluorescent lamps or similar light sources, a per-wavelength comparison of film sensitivity and spectral output is necessary to determine the correct filters for color temperature balance.

Accepted convention for evaluation of light sources, in regards to filter requirements for color balance adjustment, utilizes the reciprocal of the color temperature, which is referred to as microreciprocal degrees or mireds, when multiplied by one million. This approach is useful because a given sum of reciprocal units corresponds approximately to the same color difference for most light sources that emit a visible spectrum (in the range from 1000 K to 10,000 K). For instance, a color conversion filter that produces a 100 K color temperature decrease in a 3200 K light source will produce a decrease of about 1000 K in a 10,000 K light source. Converting these values to mireds:

(1/3200 K) x 1,000,000 = 313 mireds

(1/3100 K) x 1,000,000 = 323 mireds

323 mireds (3100 K) - 313 mireds (3200 K) = 10 mireds

and

(1/10,000 K) x 1,000,000 = 100 mireds

(1/9000 K) x 1,000,000 = 111 mireds

111 mireds (9000 K) - 100 mireds (10,000 K) = 11 mireds

It is apparent that although the degree differential between conversion of the 10,000 K and 3200 K light sources is 1000 K and 100 K respectively, the actual filtration difference is virtually the same when compared as mired units (10 versus 11 mireds).

Recently, the term reciprocal megakelvins (1/MK) has been used by Kodak and others to replace mireds. The reciprocal color temperature expressed in reciprocal megakelvins has the same value as mireds, but the value is determined by first expressing the color temperature in megakelvins (1 MK = 1,000,000 K) and taking the reciprocal. For example, a 5500 K light source can be represented as:

0.0055 MK

Taking the reciprocal:

1/0.0055 MK = 182 MK-1 = 182 Mireds

Filters designed to modify the effective color temperature of a light source can be defined in terms of their reciprocal shift value defined by the expression:

Reciprocal Shift Value = 1/T(2) - 1/T(1)

Where T(2) is the color temperature of light that has passed through the color balance filter and T(1) is the color temperature of the original light source. For example, if the color temperature of a microscope tungsten-halogen lamp is to be corrected for daylight-balanced film, the equation to calculate the reciprocal shift value would be:

1/0.0055 - 1/0.0032 = 182 - 313 = -131 MK-1

In this example, the reciprocal shift value is -131 MK-1. Notice that the sign of the reciprocal shift value is negative, which occurs when a conversion or balancing filter raises the color temperature of a light source. Conversely, when a conversion or balancing filter lowers the color temperature of a light source, the reciprocal shift value is a positive number.

Almost all indoor/tungsten films have been designed to respond with the correct color balance when illuminated by light having a color temperature of 3200 K. Under these circumstances, colors on the film will match those of the observed image. These films are referred to as type B indoor films and include the Ektachrome and Fujichrome tungsten-balanced films. Type A indoor films respond to the slightly higher color temperature of 3400 K, and include tungsten-balanced Kodachrome 40T as an example of this type of film. A color temperature of approximately 5500 K is required to match the color-balance design of all outdoor or daylight film.

One of the primary tasks in photomicrography is ensuring that the color temperature of light reaching the film is properly matched to the color temperature for which the color film has been designed. The microscope almost always uses a tungsten, or more likely a tungsten halogen bulb, as the source of light. Most specimens, with the exception of fluorescing specimens, do not emit their own light. Fluorescence equipment may use mercury or xenon burners to excite the specimen to fluoresce, which often requires matching color balance with a daylight type film.

Approximate Color Temperatures
of
Common Light Sources
Daylight Sources Color Temperature
(K)
Reciprocal
Megakelvins
(MK-1)
Skylight 12000 to 18000 83 to 56
Overcast Sky 7000 143
Noon Sun/Clear Summer Sky 5000 to 7000 200 to 143
Noon Sun/Clear Winter Sky 5500 to 6000 182 to 167
Photographic Daylight 5500 182
Noon Sunlight
(Date Dependent)
4900 to 5800 204 to 172
Average Noon Sunlight
(Northern Hemisphere)
5400 185
Sunlight at 30-Degree Altitude 4500 222
Sunlight at 20-Degree Altitude 4000 250
Sunlight at 10-Degree Altitude 3500 286
Sunrise and Sunset 3000 333
Artificial Sources Color Temperature
(K)
Reciprocal
Megakelvins
(MK-1)
Electronic Flash 5500 to 6500 182 to 154
Blue-Coated Flash Bulbs 5500 to 6500 182 to 154
Xenon Burner 6000 167
White Flame Carbon Arc 5000 200
Zirconium Flash Bulbs
(AG-1 & M3)
4200 238
Warm White Fluorescent Tubes 4000 250
Aluminum-Filled Flash Bulbs
(M2, 5, & 25)
3800 263
500-Watt 3400 K Photoflood 3400 294
500-watt 3400 K Tungsten
Photolamp
3200 313
12 Volt/100 Watt
Tungsten-Halogen @ 9 Volts
3200 313
12 Volt/50 Watt
Tungsten-Halogen @ 9 Volts
3200 313
6 Volt/20 or 30 Watt
Tungsten-Halogen @ 5.5-6 Volts
3200 313
200-Watt Household Lamp 2980 336
100-Watt Household Lamp 2900 345
75-Watt Household Lamp 2820 354
40-Watt Household Lamp 2650 377
Gaslight 2000 to 2200 500 to 455
Candlelight
(British Standard)
2900 345

Table 1

How does the microscopist ensure that the color temperature of light reaching the film matches the film's design? The temperature of the light emanating from the heated coil of the halogen bulb is dependent on the voltage sent through the bulb to heat its filament. Tungsten and tungsten-halogen lamps emit a continuous spectrum of energy that is manifested by a relatively constant output for each wavelength (Figure 2). A majority of the energy emitted by these lamps is in the long wavelength part of the spectrum (red and higher), and they subsequently produce a large amount of heat that is not useful for optical microscopy. In fact, about 90 percent of the energy emitted by tungsten and tungsten-halogen lamps is released in the form of infrared radiation and heat. The visible spectrum of a typical tungsten lamp is illustrated in Figure 2 for three color temperatures. Note that the spectral distributions are similar for each color temperature, with the ratio of blue to red increasing as color temperature is increased by raising the voltage applied to the lamp.

Almost all modern microscopes have a step-down transformer with a voltage regulator built into the base of the microscope. The voltage produced by this transformer is usually controlled by a knob or wheel or a slider positioned on the base or side of the microscope. In many modern microscopes, the voltage is signified by light emitting diodes or a voltmeter directly displaying the voltage. Table 1 shows the color temperature of several common microscope bulbs and a variety of other light sources when set at particular voltages or under natural conditions. The higher the voltage setting of the microscope's step-down transformer, the higher the color temperature of the light emitted. As the voltage is raised, the white light becomes more bluish; as the voltage is reduced, the light becomes more reddish-yellow. Once the voltage for color photomicrography has been correctly set, do not use the voltage regulator to adjust brightness, because such an adjustment will affect the color temperature.

The test of properly balanced light, matched to the film's design, is to have the clear background of a photomicrograph appear white. A bluish background indicates too high a color temperature, while a yellowish background signifies too low a color temperature.

To facilitate the correct setting for photomicrography, many modern microscopes have a photovoltage button that, when pressed, automatically sets the 12 volt 100-watt halogen lamp at 9 volts or the 6 volt 20-watt halogen lamp at 5 to 6 volts to deliver light approximating 3200 Kelvin.

When using black/white films (color temperature is not relevant here), changing the voltage going to the microscope lamp will change the intensity of the light. Raising the voltage in this instance will increase intensity and shorten exposure, whereas lowering the voltage will reduce intensity and result in longer exposures.

While the most common bulbs (12 volt, 100-watt halogen; or 6 volt 20-watt or 30-watt halogen) can be set to yield a color temperature close to 3200 Kelvin (to match the color balance of indoor Type B films), none of these bulbs (except the xenon burner) can radiate light suitable for daylight balanced films. In order to produce light simulating daylight quality, a color conversion filter must be placed in the light path, either on the light port of the microscope or in a built-in holder. The most common conversion filter (producing big jumps in color temperature) is the Kodak 80A filter (3200 Kelvin to 5500 Kelvin) or its relatives 80B, 80C, 80D (see Table 2 and Figure 3). For Olympus microscopes, the equivalent daylight-balanced filter is called the LBD filter, and for Nikon microscopes the filter is termed the NCB filter. The visible absorption spectra for the Kodak 80-series conversion filters are illustrated in Figure 3. These filters display an absorption maximum centered in the 600-650 region of the visible spectrum, which includes most of the yellow and red wavelengths. The 80A filter has the highest extinction coefficient and thus, by absorbing more red and yellow light, will produce the greatest shift in effective color temperature (see Table 2) followed by the 80B, 80C, and 80D.

Color Temperature Conversion Calculator

Use our color temperature conversion calculator to determine the appropriate filters for converting microscope illumination from one color temperature to another. Simply choose the starting color temperature and the desired final color temperature from the pull-down menus, and our interactive Java calculator will automatically perform the calculation.

Interactive Java Tutorial
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For small increases in color temperature, the light blue Kodak 82-series filters (Table 2) can be used. Conversely, for small drops in color temperature, the light yellow Kodak 81-series filters are used (Table 2 and Figure 5). When attempting to convert the color temperature of a daylight-balanced microscope light source such as a xenon lamp or flash tube for use with tungsten-balanced color film, use the amber Kodak 85-series filters. Although it is far more practical to utilize a microscope equipped with a tungsten-halogen light source, especially for critical photomicrography, these filters will serve in cases where it is impossible to use other lamps.

Exposure Compensation with Color Conversion and Balancing Filters
Filter
Changes Color Temperature
From To
Film Exposure
Increase
(F-stops)
Reciprocal Shift
Value (MK-l)
80A 3200K 5500K Daylight 2 -131
80B 3400K 5500K Daylight 1 2/3 -112
80C 3800K 5500K Daylight 1 -81
80D 4200K 5500K Daylight 1/3 -56
81 - -100K Tungsten/Daylight 1/3 9
81A - -200K Tungsten/Daylight 1/3 18
81B - -300K Tungsten/Daylight 1/3 27
81C - -400K Tungsten/Daylight 1/3 36
81D - -500K Tungsten/Daylight 2/3 45
81EF - -650K Tungsten/Daylight 2/3 59
82 - +100K Tungsten/Daylight 1/3 -9
82A - +200K Tungsten/Daylight 1/3 -18
82B - +300K Tungsten/Daylight 2/3 -27
82C - +400K Tungsten/Daylight 2/3 -36
85 5500K 3400K Tungsten
(Type A)
2/3 112
85B 5500K 3200K Tungsten
(Type B)
2/3 131
85C 5500K 3800K Tungsten 1/3 81
NCB
(Nikon)
3200K 5500K Daylight 2 -131
LBD
(Olympus)
3200K 5500K Daylight 2 -131

Table 2

These "fine tuning" filters (Kodak series 81, 82 and similar filters) useful for making smaller adjustments (100 k to 600 K) to color temperature are called color balancing filters as opposed to color conversion filters that produce large changes (several thousand kelvins) in color temperature. The values listed in Table 2 can be used as a guideline to demonstrate the effect of color balancing and conversion filters when placed in the light path. The nomograph illustrated in Figure 4 can also be used to determine the appropriate filter to be chosen to go from a known starting color temperature to the desired color temperature. To use this graph, place a straight edge ruler connecting the color temperature of the original source to that of the converted source. The point crossed on the central axis by the ruler identifies the necessary filter to achieve the color conversion. A more convenient method of determining the necessary color temperature conversion filter for color balance adjustment employs our Color Temperature Conversion Calculator, which calculates the appropriate filter when the proper starting and final color temperatures are selected from a pull-down menu.

Interactive Java Tutorial
Color Temperature Nomograph
Use our Java-powered nomograph to determine color balancing and correction filters necessary for color temperature adjustment. 

The Kodak 82-series filters, light blue in color, are useful for making small incremental increases to the color temperature of light sources that produce a color balance less than 3200 K to 3400 K. Filters of this type do not actually change the color temperature of the light source, but are useful in simulating a higher color temperature for the purposes of photomicrography. There are four filters in this series: 82, 82A, 82B, and 82C (see Table 2), and each successive filter in the series raises the color temperature by an additional 100 K increment. For example, if a light source has a color temperature of 3000 K (often found in older microscopes with a tungsten lamp), the microscopist could adjust the apparent color temperature to 3200 K with an 82A filter for use with type B tungsten-balanced film, or to 3400 K with an 82C filter for use with type A film. These filters should be an essential part of any photomicrographer's toolkit.

In situations where the color temperature of the light source is too high for a particular film, Kodak offers the 81-series filters. These filters are light yellow in color and produce incremental decreases in color temperature in a similar, but opposite manner from the 82-series filters. Because color temperature in microscope light sources is only rarely too high, these filters are seldom used in photomicrography. An exception to this is the application of 81-series filters to fine tune photomicrographs produced on tungsten-balanced film when using a daylight illumination source, such as a xenon lamp or electronic flash tube.

Some microscopes are equipped with a filter termed a daylight blue filter. This is not a filter designed for photomicrography, but is meant to produce a gray-blue background to the field of view for comfortable observation. Always remove daylight blue filters during photomicrography sessions, or when attempting to fine tune a light source with color balancing filters.

Color balancing filters and color conversion filters can be obtained as glass filters (from camera stores or microscope manufacturers) of various diameters or as the relatively inexpensive Kodak Wratten filters, that come in thin, lacquered gelatin squares 2" or 3" size. Wratten filters are produced by dissolving suitable organic dyes in liquid gelatin and coating the surface of an optical glass plate with a thin film of the solution. After drying, the gelatin film is stripped from the glass plate and coated with lacquer. Gelatin filters prepared in this manner have a thickness of 0.1 millimeter 0.01 millimeter, and exhibit a uniform thickness that is suitable for precise work in optical microscopy with negligible effect on image quality and no increase in optical path length.

Using a film that has not been correctly balanced for the light source color temperature in photomicrography can lead to unusual color shifts, resulting in unnatural hues that do not faithfully reproduce the colors seen in the microscope. The photomicrographs presented in Figure 5 demonstrate the proper use of color balance between film emulsions and microscope illumination sources. In the center (Figure 5(b)), is a photomicrograph of a thin section of cabbage root infested with the club-root soil-borne fungus Plasmodiophora bassicae. The specimen was stained with a quadruple mixture designed for plant tissue and photographed under a 3200 K light source (tungsten-halogen lamp) using Fujichrome 64T, a tungsten-balanced transparency (reversal) film. On the left (Figure 5(a)) is the same viewfield photographed using Fujichrome Velvia, a daylight-balanced film, but with the same 3200 K tungsten-halogen lamp. Note that all hues are shifted to lower wavelengths and the overall image has a definite yellow cast. The photomicrograph on the right (Figure 5(c)) was produced with the same microscope, but using a daylight-balanced flash tube for a light source, and Fujichrome 64T film. Under these conditions, the image has an overall blue cast and appears very "cool". The proper film choice for Figure 5(a) would be Fujichrome 64T (tungsten-balanced) and for Figure 5(c), it would be Fujichrome Velvia (daylight-balanced).

In modern microscopes that use Osram (or equivalent) tungsten-halogen lamps, the color temperature produced by the lamp is usually very close to 3200 K, but can decrease with age. Older microscopes, which may use a number of different 6 or 12-volt tungsten or tungsten-halogen lamps from a variety of manufacturers, often deviate (sometimes markedly) from 3200 K in color temperature. In this case, the actual color temperature of the light source is usually unknown. Other factors that may affect color temperature are optical absorption, diffusion from filters, and reflections within the microscope optical train and illumination system. When this occurs, the color temperature of illumination at the film plane may differ markedly (as much at 200 K) from that emitted by the lamp. Usually, color temperature variations induced by artifacts in the microscope optical system tend to lower (rather than raise) color temperature.

In practice, microscopists usually determine the correct filters for color temperature adjustments by trial-and-error, especially when attempting to convert illumination from an unknown value near 3200 K to 5500 K for daylight-balanced films. A good starting place for microscopes with tungsten or tungsten-halogen lamps is the Kodak 82-series light balancing filters (see Table 2). These filters have absorption spectra that display maxima with relatively high extinction coefficients in the 625-700 nanometer region (Figure 6), which covers most of the yellow and red wavelengths of the visible spectrum. By absorbing a percentage of the longer (red) visible wavelengths passing through the filter, the Kodak 82-series filters are able to increase the effective color temperature of light.

Illustrated in Figure 6 are the visible absorption spectra of the Kodak 82 and 81-series light balancing filters. The 81-series filters are able to decrease the effective color temperature of light by absorbing wavelengths in the blue (350-500 nanometers) region of the visible spectrum. An absorption maximum at 400 nanometers occurs for each of the 81-series filters, with the extinction coefficient for this maximum increasing in a periodic manner as the filter density is increased from the 81 filter through the 81EF filter. Each incremental increase in the extinction coefficient corresponds to approximately a 100 K change in color temperature (see Table 2). The same successive extinction coefficient increase is seen in the 82-series filters (Figure 6), which also corresponds to a 100 K change in color temperature for this series of filters (Table 2).

If the initial color temperature is unknown, a series of tests (much like exposure bracketing) should be conducted to determine the exact amount of filtration necessary to bring the microscope light source into balance with the color film. When using tungsten-balanced film, no other filters should be added, but when using daylight-balanced film insert a Kodak 80A, Olympus LBD, or Nikon NCB filter into the light path prior to experimenting with the Kodak 82-series filters to fine-tune the color temperature.

Start by taking a few photomicrographs with no filters in the light path to establish a baseline. Choose a specimen that displays a wide spectrum of colors and features indicative of the types of specimens that will be photographed using color film. It is also a good idea to bracket exposures to ensure the correct film exposure is being used. To do this, take photomicrographs at +2/3, +1/3, -1/3, and -2/3 f-stops centered around the recommended exposure from the microscope camera's exposure monitor. Next, add the 82 filter and take a few additional photomicrographs, followed by the 82A, 82B, 82C. It is good idea to go a step further and combine several of the filters to explore the higher end of the filtration spectrum. Do this by combining the 82 filter with either the 82A, 82B, or 82C filters, or a combination of several. Remember that exposure times will be increased when adding filters to the microscope light path, so compensate for this using the recommended exposure increases listed in Table 2. After processing the film, compare it on a suitable light table (preferably of color temperature 5500 K) and calculate the correct exposure and filter combination for the particular microscope and film. Once established, this combination should not vary and will be useful for future exposures until the microscope lamp is replaced. Remember to use the same lamp voltage for each photomicrograph to avoid introducing color balance problems.

Some higher-end photomicrographic cameras (Olympus PM-20 or PM-30) have a color temperature meter accessory (Figure 7), which can be used to read the color temperature as various filters are placed in the light path, even at low illumination levels. A light emitting diode (LED) scale indicates the reference point, against which the reading will be calibrated. The Olympus color temperature module will measure color temperature in the range of 2500 K to 10,000 K. Color temperature measurements are conducted with the specimen temporarily removed from the light path. Although expensive, this valuable option takes any guesswork out of determining exact color temperature.

Several locations are useful for adding color balancing filters to the optical path of a microscope, but these filters should always be added somewhere between the light source and the substage condenser. Some microscopes are equipped with a filter tray between the lamphouse and the field lens, which is capable of holding diffusion filters, heat-absorbing filters, and color correction filters. Other, newer microscopes, often have a built-in daylight conversion filter (LBD for Olympus and NCB for Nikon, see Table 2) housed within the base of the microscope that can be toggled into and out of the optical pathway. Many older microscopes have a filter tray built into the base of the condenser that will hold one or several color correction filters. Be careful to avoid placing the filters too close to the field diaphragm to avoid dirt and flaws on the filter surface being imaged in the specimen plane.

In conclusion, a lack of proper color temperature balance between the microscope light source and the film emulsion is the most common reason for unexpected color shifts in photomicrography. If the color temperature of the light source is too low for the film, photomicrographs will have an overall yellowish or reddish cast and will appear warm. On the other hand, when the color temperature of the light source is too high for the film, photomicrographs will have a blue cast and will appear cool. The degree of mismatch will determine the extent of these color shifts, with large discrepancies leading to extremes in color variations. Perhaps the best example (illustrated in Figure 5) is daylight film used in a microscope equipped with a tungsten-halogen illumination source without the benefit of color balancing filters. In this case, the photomicrographs will have a quite large color shift towards warmer reddish and yellowish hues. As problematic as these color shifts may seem, they are always easily corrected by the proper use of conversion and light balancing filters.

Contributing Authors

Mortimer Abramowitz - Olympus America, Inc., Two Corporate Center Drive., Melville, New York, 11747.

Michael W. Davidson - National High Magnetic Field Laboratory, 1800 East Paul Dirac Dr., The Florida State University, Tallahassee, Florida, 32310.


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