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
When by means of any of these instruments we have succeeded in forming
a single image of the two pictures, we have only, as I have already
explained, placed the one picture above the other, in so far as the
stereoscope is concerned. It is by the subsequent action of the two
eyes that we obtain the desired relief. Were we to unite the two
pictures when transparent, and take a copy of the combination by the
best possible camera, the result would be a blurred picture, in which
none of the points or lines of the one would be united with the points
or lines of the other; but were we to look at the combination with both
eyes the blurred picture would start into relief, the eyes uniting in
succession the separate points and lines of which it is composed.
Now, since, in the stereoscope, when looked into with two eyes, we see
the picture in relief with the same accuracy as, in ordinary binocular
vision, we see the same object in relief by uniting on the retina two
pictures exactly the same as the binocular ones, the mere statement of
this fact has been regarded as the theory of the stereoscope. We shall
see, however, that it is not, and that it remains to be explained, more
minutely than we have done in Chapter III., both how we see objects
in relief in ordinary binocular vision, and how we see them in the
same relief by uniting ocularly, or in the stereoscope, two dissimilar
images of them.
Before proceeding, however, to this subject, we must explain the manner
in which half and quarter lenses unite the two dissimilar pictures.
[Illustration: FIG. 17.]
In Fig. 17 is shewn a semi-lens MN, with its section M′N′. If we look
at any object successively through the portions AA′A″ in the semi-lens
MN, corresponding to _aa′a″_ in the section M′N′, which is the same as
in a quarter-lens, the object will be magnified equally in all of them,
but it will be more displaced, or more refracted, towards N, by looking
through A′ or _a′_ than through A or _a_, and most of all by looking
through A″ or _a″_, the refraction being greatest at A″ or _a″_, less
at A′ or _a′_, and still less at A or _a_. By means of a semi-lens,
or a quarter of a lens of the size of MN, we can, with an aperture
of the size of A, obtain three different degrees of displacement or
refraction, without any change of the magnifying power.
If we use a thicker lens, as shewn at M′N′_nm_, keeping the curvature
of the surface the same, we increase the refracting angle at its margin
N′_n_, we can produce any degree of displacement we require, either for
the purposes of experiment, or for the duplication of large binocular
pictures.
Public-domain text, read in full here on John Shaqi.
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