Epipolar Stereo Pair

With the Epipolar Stereo Pair operation, you will create a stereo pair from two scanned aerial photographs with overlap.

In short, the process is as follows:

Then, in the Epipolar Stereo Pair - Creation window:

When you close the Epipolar Stereo Pair - Creation window with the Exit and Show button , both input photographs will be resampled to output maps, i.e. the stereo pair is calculated. Rotation differences and possible scale differences between the photographs will be removed.

A calculated stereo pair can be viewed:

To start the Epipolar Stereo Pair operation:

Input maps and requirements:

When the Epipolar Stereo Pair is started, the Create Stereo Pair dialog box appears:

 

The operation is designed to use as input:

 

Tip: The operation can also be used on satellite images with overlap (images from different angles), but then you have to estimate the position of rotation points (explained below).

One or both of the input photographs/images may already use a georeference tiepoints, a georef direct linear, a georef orthophoto, or a georef parallel projective. However, the photographs/images may also use georef None.

The input photographs/images may use the following domains, depending on how you wish to show the stereo pair later on:

Epipolar Stereo Pair - Creation window:

After the Create Stereo Pair dialog box, the Epipolar Stereo Pair - Creation window will be opened.

 

When using satelling images:

Output stereo pair:

The dependent output stereo pair will be defined and calculated when you close the Epipolar Stereo Pair - Creation window with the Exit and Show button :

 

Each input map is rotated along the vertical axis, so that the imaginary line between principal point and transferred principal point will be exactly horizontal in the output map. Furthermore, if the input photographs had scale differences and when scaling points were specified, resampling will also increase the input map with the least pixels to the size of the other input map with the most pixels. In the output maps, rotation differences along the vertical axis and possible scale differences between the input photographs will thus be removed. This means that in the two photographs the area of overlap can be viewed in stereo. See also the Additonal Info below.

Showing the stereo pair:

A calculated stereo pair can be viewed:

You can screen digitize on the stereo pair:

 

Tip: As the output maps of a stereo pair may have a very large file size, it is advised to create Pyramid Layers for both output raster maps. This will speed up the display of the stereo pair both in the Stereo Pair - Stereoscope window and in a map window.

Additional information:

The goal of making a photo pair epipolar is that after rotation around the principal points, the corresponding lines (rows) of the resampled images contain equal places in the terrain; they are only different due to different relief displacement caused by different viewing direction. The epipolar position of the two output images is after all a situation where, ideally, the parallax of terrain objects is only present in X-direction, i.e. along image rows.

See also: