This brief introduction is written for non-photogrammetrists. It should give a rough overview about photogrammetry, its history, used instruments and some common techniques. It was not intended to be a complete reference. To get more detailled information, please choose an adequate publication from the Literature section. |
1. What is Photogrammetry |
Photogrammetry is the technique of measuring objects (2D or 3D) from photo-grammes. We say commonly photographs, but it may be also imagery stored electronically on tape or disk taken by video or CCD cameras or radiation sensors such as scanners.
The results can be:
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2. Brief History of Photogrammetry |
1851: Only a decade after the invention of the „Daguerrotypie“ by Daguerre and Niepce, the french officer Aime Laussedat develops the first photogrammetrical devices and methods. He is seen as the initiator of photogrammetry. 1858: The German architect A. Meydenbauer develops photogrammetrical techniques for the documentation of buildings and installs the first photogrammetric institute in 1885 (Royal Prussian Photogrammetric Institute). 1866: The Viennese physicist Ernst Mach publishes the idea to use the stereoscope to estimate volumetric measures. 1885: The ancient ruins of Persepolis were the first archaeological object recorded photogrammetrically. 1889: The first German manual of photogrammetry was published by C. Koppe. 1896: Eduard Gaston and Daniel Deville present the first stereoscopical instrument for vectorized mapping. 1897/98: Theodor Scheimpflug invents the double projection. 1901: Pulfrich creates the first „Stereokomparator“ and revolutionates the mapping from stereopairs. 1903: Theodor Scheimpflug invents the „Perspektograph“, an instrument for optical rectification. 1910: The ISP (International Society for Photogrammetry), now ISPRS, was founded by E. Dolezal in Austria. 1911: The Austrian Th. Scheimpflug finds a way to create rectified photographs. He is considered as the initiator of aerial photogrammetry, since he was the first succeeding to apply the photogrammetrical principles to aerial photographs. 1913: The first congress of the ISP was held in Vienna. until 1945: development and improvment of measuring (=„metric“) cameras and analogue plotters. 1964: First architectural tests with the new stereometric camera-system, which had been invented by Carl Zeiss, Oberkochen and Hans Foramitti, Vienna. 1964: Charte de Venise. 1968: First international Symposium for photogrammetrical applications to historical monuments was held in Paris - Saint Mandé. 1970: Constitution of CIPA (Comité International de la Photogrammétrie Architecturale) as one of the international specialized committees of ICOMOS (International Council on Monuments and Sites) in cooperation with ISPRS. The two main activists were Maurice Carbonnell, France, and Hans Foramitti, Austria. 1970ies: The analytical plotters, which were first used by U. Helava in 1957, revolutionate photogrammetry. They allow to apply more complex methods: aerotriangulation, bundle-adjustment, the use of amateur cameras etc. 1980ies: Due to improvements in computer hardware and software, digital photogrammetry is gaining more and more importance. 1996: 83 years after its first conference, the ISPRS comes back to Vienna, the town, where it was founded. |
3. Short description of photogrammetrical techniques |
3.1. Photographing Devices
A photographic image is a „central perspective“. This implies, that every light ray, which reached the film surface during exposure, passed through the camera lens (which is mathematically considered as a single point, the so called „perspective center“). In order to take measurements of objects from photographs, the ray bundle must be reconstructed. Therefore, the internal geometry of the used camera (which is defined by the focal length, the position of the principal point and the lens distortion) has to be precisely known. The focal length is called „principal distance“, which is the distance of the projection center from the image plane´s principal point. Depending on the availability of this knowledge, the photogrammetrist devides photographing devices into three categories:
3.1.1. Metric cameras
They have stable and precisely known internal geometries and very low lens distortions. Therefore, they are very expensive devices. The principal distance is constant, which means, that the lens cannot be sharpened when taking photographs. As a result, metric cameras are only usable within a limited range of distances towards the object. The image coordinate system is defined by (mostly) four fiducial marks, which are mounted on the frame of the camera. Terrestrial cameras can be combined with tripods and theodolites. Aerial metric cameras are built into aeroplanes mostly looking straight downwards. Today, all of them have an image format of 23 by 23 centimeters.
3.1.2. Stereometric camera
If an object is photographed from two different positions, the line between the two projection centers is called „base“. If both photographs have viewing directions, which are parallel to each other and in a right angle to the base (the so called „normal case“), then they have similar properties as the two images of our retinas. Therefore, the overlapping area of these two photographs (which are called a „stereopair“) can be seen in 3D, simulating man´s stereoscopic vision.
In practice, a stereopair can be produced with a single camera from two positions or using a stereometric camera.
A stereometric camera in principle consists of two metric cameras mounted at both ends of a bar, which has a precisely measured length (mostly 40 or 120 cm). This bar is functioning as the base. Both cameras have the same geometric properties. Since they are adjusted to the normal case, stereopairs are created easily.
3.1.3. „Amateur“ cameras
The photogrammetrist speaks of an „amateur camera“, when the internal geometry is not stable and unknown, as is the case with any „normal“ commercially available camera. However, also these can be very expensive and technically highly developed professional photographic devices. Photographing a test field with many control points and at a repeatably fixed distance setting (for example at infiniy), a „calibration“ of the camera can be calculated. In this case, the four corners of the camera frame function as fiducials. However, the precision will never reach that of metric cameras. Therefore, they can only be used for purposes, where no high accuracy is demanded. But in many practical cases such photography is better than nothing, and very useful in cases of emergency.
3.2. Photogrammetric Techniques
Depending on the available material (metric camera or not, stereopairs, shape of recorded object, control information...) and the required results (2D or 3D, accuracy...), different photogrammetric techniques can be applied. Depending on the number of photographs, three main-categories can be distinguished.
3.2.1. Mapping from a single photograph
Only useful for plane (2D) objects. Obliquely photographed plane objects show perspective deformations which have to be rectified. For rectification exists a broad range of techniques. Some of them are very simple. However, there are some limitations. To get good results even with the simple techniques, the object should be plane (as for example a wall), and since only a single photograph is used, the mappings can only be done in 2D
The rectification can be neglected, only if the object is flat and the picture is made from a vertical position towards the object. In this case, the photograph will have a unique scale factor, which can be determined, if the length of at least one distance at the object is known.
Very shortly, we will describe now some common techniques:
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Wednesday, December 19, 2007
Introduction to Photogrammetry
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