The kaleidoscope : $b its history, theory and construction. With its application to the fine and useful artsBrewster, David
Science
The kaleidoscope : $b its history, theory and construction. With its application to the fine and useful arts
Brewster, David
Kaleidoscopes
The same kind of lateral illumination may be obtained from polyhedral
cones or hemispheres of solid glass. If =A B C D=, Fig. 25, is the
section of a polyhedral cone of flint or plate glass, a portion _m
n o p_ is cut out of its base =A B=, to form an object-box for the
reception of the pieces of coloured glass, or other objects. The sides
_m n_, _m o_, _o p_, being highly polished, rays of light, either
parallel, as emanating from the sun, or diverging from artificial
sources of light, will be refracted and fall obliquely upon the faces
of the object-box, and illuminate its contents with the irregular
prismatic spectra which are formed by refraction. The apex =D C E= may,
in some cases, be cut off, and the polygonal section =D E= blackened in
order to prevent the introduction of direct light, and act as the stop
=S S= in the preceding figure.
[Illustration: FIG. 25.]
A similar effect will be obtained from a polyhedral solid, of a
hemispherical form, as shown in Fig. 26, where =A C=, =C D=, =D E=, =B
F=, =F G=, =G E=, are polished facets, by which parallel or diverging
rays immediately before it, or incident in any lateral direction, may
be refracted so as to illuminate by the prismatic rays the objects in
the box _m n o p_. The front =D E C= may have an apex, as in Fig. 25,
or may be made spherical to act as a condensing lens, the surface of
which may be blackened when necessary, for the purpose of excluding
the direct light. These illuminators may be attached in various ways
to the tube containing the reflectors, so to have a rotatory motion in
front of them.
[Illustration: FIG. 26.]
When the light is strong, a circular disk of fine grained white
paper may be advantageously placed upon the outer face _m o_ of the
object-box.
CHAPTER X.
ON THE CONSTRUCTION AND USE OF THE TELESCOPIC
KALEIDOSCOPE, FOR VIEWING OBJECTS AT A DISTANCE.
We have already seen, in explaining the principles of the Kaleidoscope,
that a symmetrical picture cannot be formed from objects placed at
any distance from the instrument. If we take the simple Kaleidoscope,
and holding an object-box in contact with the reflectors, gradually
withdraw it to a distance, the picture, which is at first perfect in
every part, will, at the distance of one-tenth of an inch, begin to be
distorted at the centre, from the disunion of the reflected images;
the distortion will gradually extend itself to the circumference, and
at the distance of eighteen inches, or less, from the reflectors, all
the symmetry and beauty of the pattern will disappear. An inexperienced
eye may still admire the circular arrangement of the imperfect and
dissimilar images; but no person acquainted with the instrument could
endure the defects of the picture, even when the slightest distortion
only is visible at the centre.
Public-domain text, read in full here on John Shaqi.
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