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 large picture for the stereoscope, we are compelled by
pictorial truth to place it at a distance from the eye equal to the
equivalent focal distance of the camera. Every picture in every camera
has the same apparent magnitude as the object which it represents;
whether it be a human figure, or the most distant landscape; and if
we desire to see it in its true relief in the stereoscope, we must
place it at a distance from the eye equal to the focal length of the
lens, whether it be an inch or a foot high. There is, therefore,
nothing gained by using large pictures. There is, on the contrary, much
inconvenience in their use. They are in themselves less portable, and
require a larger stereoscope; and we believe, no person whatever, who
is acquainted with the perfection and beauty of the binocular slides in
universal use, would either incur the expense, or take the trouble of
using pictures of a larger size.
In the beautiful combination of lenticular stereoscopes, which was
exhibited by Mr. Claudet, Mr. Williams, and others, in the Paris
Exhibition, and into which six or eight persons were looking at the
same time, binocular pictures of a larger size could not have been
conveniently used.
But, independently of these reasons, the question of large pictures
has been practically settled. No such pictures are taken by the
Daguerreotypists or Talbotypists, who are now enriching art with
the choicest views of the antiquities, and modern buildings, and
picturesque scenery of every part of the world; and even if they could
be obtained, there are no instruments fitted for their exhibition. In
the magnificent collection of stereoscopic pictures, amounting to above
a thousand, advertised by the London Stereoscopic Company, there are
no fewer than _sixty_ taken in Rome, and representing, better than a
traveller could see them there, the ancient and modern buildings of
that renowned city. Were these _sixty_ views placed on the sides of a
revolving polygon, with a stereoscope before each of its faces, a score
of persons might, in the course of an hour, see more of Rome, and see
it better, than if they had visited it in person. At all events, those
who are neither able nor willing to bear the expense, and undergo the
toil of personal travel, would, in such a panorama,—an analytical view
of Rome,—acquire as perfect a knowledge of its localities, ancient
and modern, as the ordinary traveller. In the same manner, we might
study the other metropolitan cities of the world, and travel from them
to its river and mountain scenery,—admiring its noble castles in our
descent of the Rhine,—its grand and wild scenery on the banks of the
Mississippi, or the Orinoco,—the mountain gorges, the glaciers, and the
peaks of the Alps and the Ural,—and the more sublime grandeur which
reigns among the solitudes of the Himalaya and the Andes.
Public-domain text, read in full here on John Shaqi.
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