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New trends in physics teaching, v.4; The ... - unesdoc - Unesco

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Colour<br />

I<br />

120<br />

Noon Summer Sunlight<br />

5740K<br />

--I<br />

4O F<br />

Noon W<strong>in</strong>ter Sunlight<br />

01 I I I I I<br />

400 500 600<br />

Wavelength/nm<br />

Figure 19. Sunlight at different times of the year at mid latitudes.<br />

Sources of Light<br />

We have said very little about the nature of light sources so far, because we wished to <strong>in</strong>troduce<br />

the CIE chromaticity diagram first as a means of specify<strong>in</strong>g their colour. Daylight itself is a very<br />

variable quantity, as shown <strong>in</strong> figure 19 for sunlight. North light, or the blue sky, which is sunlight<br />

scattered by small particles <strong>in</strong> the atmosphere, can exceed 7000 K colour temperature.<br />

Fluorescent light comes from mercury discharge tubes, which give only s<strong>in</strong>gle l<strong>in</strong>es <strong>in</strong> the<br />

spectrum, as shown <strong>in</strong> figure 20. Fluorescent powders <strong>in</strong>side the discharge tube modify this to<br />

give a white light spectrum.<br />

200 300 400 500 600 700<br />

Wave I e ngt h /nm<br />

Figure 20. L<strong>in</strong>e spectrum of a low pressure mercury vapour lamp.<br />

213

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