Colour Measurement and MixtureAbney, William de Wiveleslie, Sir
Science
Colour Measurement and Mixture
Abney, William de Wiveleslie, Sir
Color
The drawback to the use of prisms is that the dispersion of the red end
of the spectrum is much less than that of the blue end, and is apt to
give a false impression as to the relative luminosities of, and length
of spectrum occupied by, the different colours. In some text-books it is
told us that the diffraction grating gives us a dispersion which is in
exact relation to the wave-length. This is not true, however, as it can
only give one small portion in such relationship, and that only when it
is specially set for the purpose. The subject of diffraction is one into
which it would be foreign to our purpose to wander. We may say that for
measures such as we shall make, it is handier to employ prisms, as the
prismatic spectrum is more intense than the diffraction spectrum. This
can be readily understood when we consider the subject even
superficially. If we throw a beam of light on a grating which contains
perhaps some 14,000 parallel lines in the space of one inch in width,
the lines being ruled on a plane and bright metallic surface, and
receive the reflected beam on a screen, the appearance that is presented
is a white central spot, together with six or seven spectra of gradually
diminishing brightness on each side of it, all except the first pair
overlapping one another. That these different spectra do exist can be
readily shown by placing in the beam a piece of red glass, when
symmetrical pairs of the red part of the spectrum will be found, one of
each pair being on opposite sides of what will now be the central red
spot. Half the light falling on the grating is concentrated in this
central spot, and the remaining half goes to form the spectra; the pair
nearest the central spot being the brightest. We thus are drawn to the
conclusion that at the outside we can only have less than one-quarter of
the incident light to form the brightest spectrum we can use. With two
good prisms we use at last three-fourths of the incident light, so that
for the same length of spectrum we can get at least three times the
average brightness that we should get were we to employ a diffraction
grating.
Public-domain text, read in full here on John Shaqi.
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