Parallax: The apparent displacement of the position of a body, with respect to a reference point or system, caused by a shift in the point of observation.
Absolute Parallax: Considering a pair of aerial photographs of equal principle distance, the absolute parallax is the difference of a point is the algebraic difference of the distances of the two images from their respective photo nadirs measured in a horizontal plane and parallel to the air base.
Differential Parallax: The difference in the absolute stereoscopic parallaxes of two points imaged on a pair of photographs. This is usually employed in the determination of the differences in the elevation of objects.
Here we assume that the shadow on which the ground falls is level and that the object is vertical. The object's top must be sharply defined so that it creates a distinct image. There are many sources of error here, shadows are not always distinct, and the calculation of the sun angle is an involved process.
Ho = Ha x D
R
Where:
Ho = Height of the object;
Ha = Altitude above the surface where the photo is taken;
D = Length of the displaced image;
R = Radial distance from the photo nadir to the top of the object.
Basically, its important that you know that these techniques exist. That they can be accomplished in a practical fashion if necessary. If you ever have to do this you can always go back and cookbook it.
Parallax Height Measurement
This is the most used method of measuring heights on air photos. There are many forms of the parallax equations. Avery and Berlin give one; Paine in his book lists three: 1) for mountainous terrain; 2) for level terrain; and, 3) the short cut equation.
What I will give here is the basic form of the equation:
Ho = Ha x dP
Pb + dP
Where: Ho = The height of the object of interest;
Ha = Platform height or altitude above datum;
dP = Differential Parallax; and
Pb = Absolute Parallax.
So if the altitude of the aircraft above datum is: 1. known or can be calculated; and, 2. if, from the available stereo pairs, we can calculate the differential and the absolute parallax; then, 3. We can ascertain the heights of objects in the photos.
Important things to remember here include:
Now for a small trick. If we can assume that:
Then, we can substitute the average photobase of the stereo pairs
being used can be substituted for Pb (absolute parallax).
Let's say, as Avery and Berlin do in their book (5th. ed.) on Pg. 78 and 79; that we are going to measure the height of the Washington Monument from a stereo pair.
The nominal photo scale we have is 1:4,800. We have gone in and corrected this in the area of the monument monument to 1:4,600 at the base of the Monument. The camera focal length was 12 inches. So the flying height was what? 4,600 feet. The average photobase (P) of the stereopair is calculated to be: 4.40 inches.
Absolute stereo parallax at the base; and at the top of the monument is measured parallel to the line of flight with an engineers scale. The difference is: 2.06 in. - 1.46 in. This gives a dP of 0.60 in. So, 0.60 inches is the differential parallax of the displaced images.
Substituting these values into a form of our formula:
Ho = [H] dP
Pb + dP
Ho = 4,600 Ft. 0.60 in. = 552 feet
4.40 in. - 0.60 in.
The actual height of the Washington Monument is 555 feet. This is a
very accurate measurement for this type of exercise. For example if we
had used the nominal photo scale of 1: 4,800; instead of the corrected
1: 4,600 scale we would have gotten a height of 576 feet. A 21 foot error
as opposed to the 3 foot error we did get. It just goes to show that the
more time you put in setting up the problem and the more precise the instruments
are the better ( up to a point) the measurements that you can achieve.
Well that's essentially it for stereo and height measurement.