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
Hence, in order to find the binocular centres D, D′, D″, D‴, &c., at
any altitude, E, E′, &c., we have only to join EG, E′G, &c., and the
points of intersection D, D′, &c., will be the binocular centres,
and the lines DC, D′C, &c., drawn to C, will be the real lengths and
inclinations of the united images of the lines AC, BC.
When GO is greater than GC there is obviously some angle A, or E″GM, at
which D″C is perpendicular to GC.
This takes place when
GC
Cos. A = ————.
GO
When O coincides with C, the images CD, CD′, &c., will have the same
positions and magnitudes as the chords of the altitudes A of the eyes
above the plane GC. In this case the raised or united images will just
reach the perpendicular when the eye is in the plane GCM, for since
GC = GO, Cos. A = 1 and A = 0.
When the eye at any position, E″ for example, sees the points A and B
united at D″, it sees also the whole lines AC, BC forming the image
D″C. The binocular centre must, therefore, run rapidly along the line
D″C; that is, the inclination of the optic axes must gradually diminish
till the binocular centre reaches C, when all strain is removed. The
vision of the image D″C, however, is carried on so rapidly that the
binocular centre returns to D″ without the eye being sensible of the
removal and resumption of the strain which is required in maintaining
a view of the united image D″C. If we now suppose AB to diminish,
the binocular centre will advance towards G, and the length and
inclination of the united images DC, D′C, &c., will diminish also, and
_vice versa_. If the distance RL (Fig. 26) between the eyes diminishes,
the binocular centre will retire towards E, and the length and
inclination of the images will increase. Hence persons with eyes more
or less distant will see the united images in different places and of
different sizes, though the quantities A and AB be invariable.
While the eyes at E″ are running along the lines AC, BC, let us suppose
them to rest upon the points _ab_ equidistant from C. Join _ab_, and
from the point _g_, where _ab_ intersects GC, draw the line _g_E″, and
find the point _d″_ from the formula
_g_E″ × _ab_
_gd″_ = ———————————-.
_ab_ + RL
Hence the two points _a_, _b_ will be united at _d″_, and when the
angle E″GC is such that the line joining D and C is perpendicular to
GC, the line joining _d″_C will also be perpendicular to GC, the loci
of the points D″_d″_, &c., will be in that perpendicular, and the image
DC, seen by successive movements of the binocular centre from D″ to C,
will be a straight line.
Public-domain text, read in full here on John Shaqi.
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