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In refraction stereoscopes, invented in 1849 by David Brewster
(1781-1868), the two reproductions are viewed through two prismatic lenses,
one for each eye, which can be described as composed of two converging
lenses to which two prisms having a small refractivity angle are attached
in the front, with the edges turned towards the axis of the instrument.
The lenses give two virtual images of the two reproductions at the distance
of distinct vision which the two prisms, on deviating their incident rays,
superimpose; thus a single image is observed in a position between the
two giving the perception of rises and depressions in three dimensions.
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