The sun is a natural source of radiant energy, and its spectral radiant power distribution depends on whether the light is direct or reflected, its position in the sky, and the conditions of the atmosphere.
9 As a result, sunlight is redder at dawn and dusk than in the middle of the day, with roughly equal amounts of red, green, and blue at noon and under cloudy conditions. Sunlight is much richer in short-wavelength light than most artificial illuminants, such as tungsten and fluorescent lights, and the correlated color temperature can range from 5000 to 7000 K (sunlight incident on a horizontal surface regardless of cloud cover) to 40,000 K (clear, north sky). In
Figure 1, sunlight is represented by the International Commission on Illumination (CIE) Standard Illuminant D
65, which has a color temperature of 6504 K. For the purpose of allowing comparison between illuminants, the intensity of the D
65 light source has been normalized to the other illuminants at 555 nm.
Figure 1 illustrates that tungsten lights are especially low in short wavelength light and rich in long wavelength light (2850–3100 K), while fluorescent lights have energy-rich bands distributed throughout the visible spectrum, which are dependent on the phosphors and activators present. Fluorescent lighting has been associated with increased prevalence of hyperopia
10 and astigmatism
11 and the preponderance of longer wavelengths in artificial illuminants has been proposed as a potential cause of myopia,
12 though others have not found any effect.
13 Because neither tungsten nor fluorescent lights replicate the spectral output or intensity of the sun, short-wavelength sensitive cone stimulation may be compromised at normal indoor illumination levels, particularly by tungsten bulbs.