The stereoscope : $b its history, theory, and construction, with its application to the fine and useful arts and to educationBrewster, David
History
The stereoscope : $b its history, theory, and construction, with its application to the fine and useful arts and to education
Brewster, David
Stereoscope
If we take a reading-glass whose diameter is not less than two inches
and three quarters, and look through it with both eyes at a binocular
picture in which the right-eye view is on the left hand, and the
left-eye view on the right hand, as in the ocular stereoscope, we shall
see each picture doubled, and the degree of separation is proportional
to the distance of the picture from the eye. If the distance of the
binocular pictures from each other is small, the two middle images of
the four will be united when their distance from the lens is not very
much greater than its focal length. With a reading-glass 4½ inches in
diameter, with a focal length of two feet, binocular pictures, in which
the distance of similar parts is _nine_ inches, are united without
any exertion of the eyes at the distance of eight feet. With the same
reading-glass, binocular pictures, at the usual distance of 2½ inches,
will be united at the distance of 2¼ or even 2½ feet. If we advance the
reading-glass when the distance is 2 or 3 feet, the picture in relief
will be magnified, but, though the observer may not notice it, the
separated images are now kept united by a slight convergency of the
optic axes. Although the pictures are placed so far beyond the anterior
focus of the lens, they are exceedingly distinct. The distinctness of
vision is sufficient, at least to long-sighted eyes, when the pictures
are placed within 16 or 18 inches of the observer, that is, 6 or 8
inches nearer the eye than the anterior focus of the lens. In this
case we can maintain the union of the pictures only when we begin to
view them at a distance of 2½ or 3 feet, and then gradually advance
the lens within 16 or 18 inches of the pictures. At considerable
distances, the pictures are most magnified by advancing the lens while
the head of the observer is stationary.
9. _The Camera Stereoscope._
The object of this instrument is to unite the transient pictures of
groups of persons or landscapes, as delineated in two dissimilar
pictures, on the ground-glass of a binocular camera. If we attach
to the back of the camera a lenticular stereoscope, so that the two
pictures on the ground-glass occupy the same place as its usual
binocular slides, we shall see the group of figures in relief under
every change of attitude, position, and expression. The two pictures
may be formed in the air, or, more curiously still, upon a wreath of
smoke. As the figures are necessarily inverted in the camera, they
will remain inverted by the lenticular and every other instrument but
the opera-glass stereoscope, which inverts the object. By applying
it therefore to the camera, we obtain an instrument by which the
photographic artist can make experiments, and try the effect which will
be produced by his pictures before he takes them. He can thus select
the best forms of groups of persons and of landscapes, and thus produce
works of great interest and value.
10. _The Chromatic Stereoscope._
Public-domain text, read in full here on John Shaqi.
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