Theory for the determination of differences in elevation
of points on the aerial photograph by measuring the x-parallax
is next studied. The various parallax measuring instruments
are discussed and demonstrated, After learning the fundamentals
of operating the various height finders, parallax bars, or stere-
ometers, the trainee works with a set of photographs and the ac-
companying topographic map. Differences in elevation of given
points are determined and compared with the differences as rep-
resented on the topographic map. When the trainee has become
adept in this technique the effect of tilt in the stereoscopic
model is analyzed, using the technique in conjunction with the
topographic base map. The parallax bar 1s then used to make
three-point dip and strike determinations and results are com-
pared to measurements previously made in the field with the
Brunton compass or plane table and alidade, Measurements of
the thickness of stratigraphic units are also made, using the
parallax bar.
Vertical exaggeration is demonstrated by using the Stereo-
slope Comparator, This instrument, developed by the U, S. Geo-
logical Survey, 1s designed to compute the inclination of planar
features in a stereoscopic model using as its principal of opera-
tion a vertical exaggeration constant for a given operator under
Specific viewing and photographic conditions. After thorough
orientation in operation of this instrument the geologists
measure the strike and dip of strata as expressed in the aerial
photographs and compare the results with measurements of the same
features performed by field methods. By this demonstration the
trainee is made aware of the effects of vertical exaggeration
and why they must be considered by the photo-interpreter and
specifically by the geologist whose work depends on correct in-
terpretation and visualization of dipping strata.
Two methods for properly annotating the aerial photographs
are shown, 1) annotation of the entire area of alternate pho-
tographs in a flight line and, 2) annotation of the right half
of every photograph in the flight line. The latter method
permits a continuity of lines from one stereoscopic model to
the next.