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Figure 1: The region of the sun's spectrum that spans the range from ultraviolet (UV) to infrared (IR). Different portions of the sun's energy are absorbed in the atmosphere, water, and glass. Human daylight vision is most effective in the blue-green (around 550 nm) where the sun's energy spectrum is in the region of its maximum. Figure 2 shows the spectrum of the sun along with those of a tungsten lamp and a candle flame, both incandescent light sources where incandescence refers to light produced by the temperature of an object. In a candle, the wax is melted by the heat of the flame, flows up the wick and is vaporized. Combustion raises the temperature of the carbon particles to incandescence and causes the emission of the yellow color. As shown in Fig. 2 the maximum in the visible spectrum is at the long wavelength, red, end.
Figure 2: Energy spectrum in the visible region for the sun, tungsten lamp, and candle flame In the tungsten lamp, the electric current runs through the filament which becomes hot and radiates. As with the candle some of the radiation is in the visible but most is in the infrared (IR). To keep the tungsten filament from burning or melting, the glass bulb is filled with a mixture of argon and nitrogen gases that does not react with tungsten. Fluorescent lamps operate by a different principle from incandescence, a gas discharge. A glass tube is filled with mercury vapor and others, such as sodium, and the electrodes are connected to an alternating current (AC) source. The electric source ionizes the atoms in the tube which emit light primarily in the UV. The inside of the tube is coated with phosphors which absorb UV light and produce visible light. Consequently, fluorescent tubes have an energy spectrum with a broad spectrum, similar to the tungsten lamp, and a series of sharp intense peaks in the red, blue, and green. The intense green line (mercury vapor) at 546 nm is used to calibrate spectrometers.
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