A SYSTEM FOR THE NORMAL CASE OF CLOSE-RANGE
PHOTOGRAPHY WITH TERRESTRIAL CAMERA
Ojuz MÜFTÜOGLU - Cankut ÓRMECI
Surveying Department of Civil Engineering Faculty
istanbul Technical University, istanbul - Türkiye
ABSTRACT
The normal case of close-range photograph is realized by using WILD P32 terrestrial
camera in which the base is changeable and known. With a system that has been
developed for this purpose, photographs have been obtained by using a single metric
camera which is capable of sliding on two steel bars ranging from 1 mm to 400 mm.
While the base can vary from 1 mm to 400 mm if the photographs are taken 12 cm base,
it will provide technical characteristics of WILD C12 and C120, and it allows user
to obtain drawing outputs of 1/50, 1/100 and smaller scales by using WILD A40
Autograph. Also if photographs are to be taken at 400 mm base, larger-scale drawing
outputs can be achieved. This system has been successfuly in use in the close-range
photogrammetric applications, such as archaelogical and architectural projects.
KEY WORDS: Close-range photogrammetry, Terrestrial Camera, Design
l. INTRODUCTION
Many methods of close-range photogrammetry
require special equipment, both for taking
of the photographs and their subsequent
measurement, and the availability of these
Special cameras and plotting instruments
has allowed the full potential of close-
range photogrammetry to be realised in
many branches of science and engineering.
Non-topographic applications of photog-
rammetry are made in the areas of medicine.
dentistry, architecture, human locomotion,
archaelogy, experimental analysis of
structures, hydraulics, ship building,
animal husbandry, deformations of dams,
glacier and earth slide movements, vehicle
motion, missile tracking, accident recon-
Struction, and underwater events, to name
but a few. In most of the applications
listed above, a ground-based camera is
used. Close range metric cameras include
single cameras and stereometric cameras.
There are three main problems to be resolved
in ground-based cameras. These are
respectively camera position, camera-
object distance, and the orientation of
the camera image plane. Single cameras,
in original using, mounts directly on the
telescope of a theodolite to overcome these
problems. On the other hand, because the
camera position can be determined precisely
and the orientation of the axis of the
camera set to any desired direction, much
more can be known of the relative and
absolute orientation of a pair of photograrhs
in close-range photogrammetry than in
aerial work, and this offers advantages.
Some situations call for stereometric
cameras, where the axes of the two cameras
are parallel, and a special instrument has
been developed and designed to exploit
fully this known geometry by using one
single metric camera.
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