Approximate Correlated Color Temperature for Various Light Sources

Source Degrees K
Artificial Light
Match Flame 1700
Candle Flame 1850
40-Watt Incandescent Tungsten Lamp 2650
75-Watt Incandescent Tungsten Lamp 2820
100-Watt Incandescent Tungsten Lamp 2865
500-Watt Incandescent Tungsten Lamp 2960
200-Watt Incandescent Tungsten Lamp 2980
1000-Watt Incandescent Tungsten Lamp 2990
3200-Degree Kelvin Tungsten Lamp 3200
Molarc "Brute" with Yellow Flame Carbons & YF-101 Filter (approx.) 3350
"C.P." (Color Photography) Studio Tungsten Lamp 3350
Photoflood or Reflector Flood Lamp 3400
Daylight Blue Photoflood Lamp 4800
White Flame Carbon Arc Lamp 5000
High-Intensity Sun Arc Lamp 5500
Xenon Arc Lamp 6420
Daylight
Sunlight: Sunrise or Sunset 2000
Sunlight: One Hour After Sunrise 3500
Sunlight: Early Morning 4300
Sunlight: Late Afternoon 4300
Average Summer Sunlight at Noon (Washington, D.C.) 5400
Direct Mid-Summer Sunlight 5800
Overcast Sky 6000
Average Summer Sunlight (plus blue skylight) 6500
Light Summer Shade 7100
Average Summer Shade 8000
Summer Skylight Will Vary from 9500 to 30000

NOTE: Sunlight is the light of the sun only. Daylight is a combination of sunlight plus skylight. The values given are approximate because many factors affect color temperature. OUTDOORS: the sun angle, and the conditions of the sky-clouds, haze, dust particles-raise or lower the color temperature. INDOORS: lamp age (and blackening), voltage, type of reflectors and diffusers affect tungsten bulbs all of these can influence the actual color temperature of the light. Usually a change of 1 volt equals 10 degrees Kelvin. But this is true only within a limited voltage range and does not always apply to "booster voltage" operation, since certain bulbs will not exceed a certain color temperature regardless of the increase in voltage.

 
about Color Temperature and Light sources
 
Standards of Luminous Intensity and
Their Color Temperatures
Source Color Temperature
(Kelvin)
Standard British candle
Hefner
Harcourt pentane
Acetylene
Incandescentcarbon (4 watts/candle)
Incandescent tungsten (1.25 watts/candle)
Freezing point of platinum
1930
1880
1920
2415
2080
2400
2042
 
 
 
 
Selected Practical Sources of Illumination and Their Color Temperatures
Source Color Temperature 
(Kelvin)
Mired
Value
Sunlight (mean noon)
Skylight
Photographic.Daylight
Crater of carbon arc (ordinary hard-cored)
White-flame carbon arc
Flashcube, magicube or flipflash
High-intensity carbon arc (sun arc)
Clear zirconium wire-filled flash
Clear aluminum wire-filled flash
500-watt (photoflood) approx. 34.0 lumens/watt
500-watt (3200 K photographic) approx 27.0 lumens/watt
200-watt (general service) approx 20.0 lumens/watt
100-watt (general service) approx 17.5 lumens/watt
75-watt (general service) approx 15.4 lumens/watt
40-watt (general service) approx 11.8 lumens/watt
5400
12000 to 18000
5500
4000
5000
4950
5500
4200
3800
3400
3200
2980
2900
2820
2650
185
83 to 56
182
250
200
202
182
238
263
294
312
336
345
353
377

 

According to Kodak:

 

 

Mired System for light conversion

                                    1.000.000
Mired value=   -------------------------------
                          color temperature in kelvin
 

Mired Values of Color Temperatures from 2000-6900 K
K 0 100 200 300 400 500 600 700 800 900
2000
3000
4000
5000
6000
500
333
250
200
167
476
323
244
196
164
455
312
238
192
161
435
303
233
189
159
417
294
227
185
156
400
286
222
182
154
385
278
217
179
152
370
270
213
175
149
357
263
208
172
147
345
256
204
169
145
 
 
T1 represent the color temperature of the original light source. represent the color temperature of the light through the filter.Using some filters, like Kodak light balancing filters, we can modify the effective color temperature. Giving to each filter a mired shift value, represented by the expression (1/T2 - 1/T1)*106
 either positive or negative, you can change the color temperature. Using yellowish filters, the mired value increases, having a positive mired shift value, resulting lower color temperature.Using bluish filters, the mired value decreases, having a negative mired sift value, resulting higher color temperature.
The above nomograph simplify to theory, showing the proper conversion filter. To find the requested filter (the mired shift value), place a straightedge on the points corresponding to the color temperature of the source,  T1,  and the color temperature of the desired sourceT2

 

Here are two depictions of the color temperature scale from 1000K to 10000K. They use two different mappings from CIE x,y coordinates to the surface of the RGB color cube. The first maps the "E" point, 1/3,1/3 to 1,1,1. The second maps the x,y coordinates of CIE standard illuminant C, 0.310, 0.316 to 1,1,1. The second mapping gives a more pleasing rendition as it passes through "white" at a higher temperature. Compare these with the color scales in e.g. the Cambridge Encyclopedia of Astronomy, Chapter 3.