E DLKOTE s 1T
PPO OGRANMPILIKY, Vol. AZEA
i
Communication to
VIII International Congress for Photogrammetry
Reprint from
Svensk Lantmateritidskrift
Congress Number 1956
Commission 11
DEVICE FOR MEASUREMENTS OF PARALLAXES
By
Gunnar Simonsson
The devices usually used for parallax measurements by means of
mirror or pocket stereoscopes in aerial photographs are: Stereometers
(or parallax bars) and parallax wedges.
The stereometer is a micrometer screw to which are attached two
glass plates carrying the measuring marks. By screwing the micrometer
the two marks can be set to identical details in the two photographs, the
distance between these details — the horizontal parallax — being read
on a reading drum.
The parallax wedge consists of two non — parallel lines engraved on
the bottom of a glass plate. Corresponding parts of the lines are brought
to coinside with identical details in the photographs. The horizontal pa-
rallaxes can be read on a scale close to one (or both) of the lines.
Fundamentally the device here described is a type of parallax wedge,
the lines being substituted by rows of dots. The rows, instead of being
straight lines, form the systems of points shown by Figure 1. As the
two lines of the wedge are not parallel, consequently, the two point sys-
tems in Figure 1 have to be unequally shaped. The point row starts with
the first point in the U-shaped point group at the top of the system,
(See Figure 4), follows the sequences of point groups, and ends with
the last point in the point group at the bottom of the system. Each point
in the left system corresponds to a point in the right system. A point
step represents a parallax difference of 1/10 millimeter. Thus each
point group represents a parallax difference of 1 millimeter and, con-
sequently, the whole system, consisting of 20 point groups, allows mea-
suring parallax differences up to 20 millimeters. s
There are two obvious advantages of this arrangement of the points:
l. All points required for the parallax measurements are concentrated
Within a small area, which means that the plate can be attached to the
Stereoscope at the beginning of the work and need not then be remo-
ved. (Only small adjustment of vertical parallaxes may be needed.)
A EL NS esci TO MA ed C APRI DE C