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

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

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Colour<br />

Colour<br />

R.D. EDGE.<br />

Colour, like pitch <strong>in</strong> music, is a perceptual quantity - what we see, light from objects, is observed<br />

by the human eye and <strong>in</strong>terpreted by the bra<strong>in</strong>. Physics represents only a part of this, but it is the<br />

part most easily dealt with. Nevertheless, teach<strong>in</strong>g art students and other non-physicists the<br />

physical basis of colour and its relationship to the appearance of pigments, colour film and colour<br />

television presents no easy task - an artist perceives colour <strong>in</strong> quite a different way from a dye<br />

chemist or a physicist. Because colour overlaps the prov<strong>in</strong>ces of <strong>physics</strong>, psychology and eng<strong>in</strong>eer<strong>in</strong>g,<br />

the term<strong>in</strong>ology used is mixed and confus<strong>in</strong>g. Emphasis wil be laid on these differences to<br />

try to avoid this problem.<br />

LIGHT<br />

Thomas Young first demonstrated light to be a wave phenomenon <strong>in</strong> 1801 by show<strong>in</strong>g that the<br />

troughs and crests of two overlapp<strong>in</strong>g beams of light can <strong>in</strong>terfere to produce visible dark and<br />

bright bands. In 1864 Maxwell showed light to be a form of electromagnetic radiation. Long<br />

before <strong>New</strong>ton’s Opticks [ 11 , it was known that white light could be spread <strong>in</strong>to a spectrum of<br />

colours by a glass prism. <strong>The</strong> actual range of wavelengths which can be seen is small - from 360<br />

to 740 nm (1 nanometre = lo-’ m), less than a factor of two, an octave. Although we shall<br />

describe light as a wave <strong>in</strong> our discussions of colour and <strong>in</strong> its path from the source to the eye,<br />

modern <strong>in</strong>vestigations show its production and detection can often be more easily described by<br />

particle behaviour - the ‘photon> of light. Once we have split the light emitted by, or reflected<br />

from, an object <strong>in</strong>to its component wavelengths, as by a prism, and measured how much of each<br />

there is, thus obta<strong>in</strong><strong>in</strong>g the <strong>in</strong>tensity spectrum, we have virtually completed the physical specification<br />

of that light - there is little else to discuss. (We are not <strong>in</strong>terested <strong>in</strong> polarization - the<br />

vibration direction of the light.) However, the colour which we perceive wil also depend on the<br />

surround<strong>in</strong>gs of our object, how bright the illum<strong>in</strong>ation is and other factors.<br />

Light is energy, and as such may be converted <strong>in</strong>to other forms of energy - such as heat (as<br />

we notice, sitt<strong>in</strong>g <strong>in</strong> the sun) or electrical energy, as by a photocell. We are <strong>in</strong>terested <strong>in</strong> the<br />

illum<strong>in</strong>ation of objects and wish to measure the flow of the light energy onto objects we observe.<br />

<strong>The</strong> radiance, or flow of light energy per unit area (sometimes called the flux) is measured <strong>in</strong><br />

physical units of watts per square metre, the watt be<strong>in</strong>g a joule per second.<br />

193

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