Colour Measurement and MixtureAbney, William de Wiveleslie, Sir
Science
Colour Measurement and Mixture
Abney, William de Wiveleslie, Sir
Color
red and infra-red, and it is owing to the heating of the paint by these
rays that the image might be at first slightly brighter than the
background, and subsequently darker.
There is another way in which the existence of both the ultra-violet and
infra-red rays can be demonstrated, and that is by means of photography.
If we place an ordinary photographic plate in the spectrum and develop
it, we shall find that besides being affected by the blue and violet
rays, it is also affected by the rays beyond the violet, the energy of
these rays being capable of causing a decomposition of the sensitive
silver salt. If quartz prisms and lenses be used, and the electric light
be the source of illumination, the ultra-violet spectrum will extend to
an enormous extent. A more difficult, but perhaps even more interesting
means of illustrating the existence of the infra-red rays, and first due
to the writer, can be made by means of photography. It is possible to
prepare a photographic plate with bromide of silver, which is so
molecularly arranged that it becomes capable of being decomposed not
only by the violet and blue rays, but also by the red rays, and by those
rays which have wave-lengths of nearly three times that of the red rays.
It would be inappropriate to enter into a description of the method of
the preparation of these plates. Those who are curious as to it will
find a description in the Bakerian lecture published in the
Philosophical Transactions of the Royal Society for 1881. With plates so
prepared it has been found possible to obtain impressions in the dark
with the rays coming from a black object, heated to only a black heat.
That these dark rays possess greater energy or capacity for doing work
of some kind than any other rays of the spectrum, can be shown by means
of a linear thermopile (Fig. 4), if it be so arranged as to allow only a
narrow vertical slice of light to reach its face.
Fig. 4.--The Thermopile.
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