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FILM DEFORMATION IN NON METRIC CAMERAS UNDER WEAK GEOMETRIC CONDITIONS - AN
UNCORRECTED DISASTER?
Dr. Stuart Robson, Engineering Surveying Research Centre,
City University, Northampton Square, London ECIV OHB.
ISPRS Commission V/2.
Abstract:
Whilst multi-station bundle adjustments are almost universally applied to high precision photogrammetric surveys for
engineering purposes, the use of often as few as two camera stations for less stringent architectural and archaeological
surveys is common. The effect of in-camera deformations has been well documented in the former case, but for simpler
geometric situations the effects and magnitudes of unmodelled distortions on the computed object space coordinates are
less well documented.
Self compensating effects of in-camera deformation within a strong network adjustment are illustrated with reference to
experiments carried out using a range of film type and camera back permutations. The number of camera stations
contributing to the network was then reduced and a range of film deformation correction techniques applied. By comparing
results from both series of adjustments the effect of network geometry and film deformation on the computed object space
coordinates was investigated.
Results show that whilst root mean square object space discrepancies can vary minimally for adjustments incorporating
differing film deformation corrections and a given network geometry, significant trends due to uncorrected film
deformation can be present in the computed object space coordinates .
KEY WORDS: Accuracy, Calibration, Close-range, Film, Non-metric.
LIntroduction.
Photogrammetry is used to measure dimensions and
positions of objects according to some reference system
or datum. This analysis sets out to investigate the influence
of photographic film deformation and its correction, based
on reseau measurement, on the object space coordinates
derived by photogrammetric adjustment.
The influences of un-modelled image deformations on
derived object coordinates have been shown to be largely
self compensating in strong network multi-station bundle
adjustments (Fraser 1984, Wester-Ebbinghaus 1988).
However, the majority of photogrammetric surveys
intended for commercial purposes, for example
architectural surveys, generally try to achieve
photographic coverage of the object of interest using a
minimum number of stereo pairs. This means that not only
are any self compensating effects reduced, but also since
there are fewer redundant measurements it is often
difficult to determine the effects of unmodelled errors.
This paper draws upon results produced during a
comprehensive series of close range calibrations in which
a variety of medium format cameras were used. Format
sizes range from 130 by 180mm to 60 by 60mm. The
experimental work begins with the knowledge that
in-plane film deformation has been minimised (Robson
1990) and that deformations occurring in the non-metric
camera used are almost an order of magnitude greater than
those attributed to in-plane film deformational factors.
2. Practical Approach.
The effectiveness of film deformation correction methods
can be investigated by conducting a photogrammetric
Survey of an array of targets with known X,Y,Z object
Space coordinates. Target positions as estimated by any
Subsequent photogrammetric adjustment based on the
Same datum may be directly compared with the original
target positions. Any differences in position introduced
either by change in network configuration or by variation
of film deformation correction can be assessed. The key
problem associated with this method is to obtain initial
X,Y,Z target coordinates at a greater level of precision
than those estimated during the photogrammetric
adjustments featuring network or film deformation
correction changes.
This analysis is concerned primarily with object
coordinate deformation in single stereopairs. One method
of deriving X,Y,Z target coordinates of suitably high
precision is to carry out a free photogrammetric
adjustment of the same target array based on a strong
network incorporating many photographs.
2.1 Test Field Design.
A test field was designed based on several factors; the
imaging abilities of a Hasselblad SWC camera, namely a
resolution of at least 50 1 mmr! over the complete format
with Technical Pan 120 film; an image measurement
magnification of 200X and 0.5 pm rms provided by the
modified ZKM measuring microscope at the National
Physical Laboratory (Oldfield 1986, Zeiss 1985) and; on
the requirement of long term durability such that the
calibration procedure could be repeated as required.
The final test field design consisted of 42 targets pinned
into a concrete wall by countersunk titanium bars and
several additional free standing targets for densification.
The starting positions of these targets could then be
derived by conventional survey to provide the "free
adjustment' datum. The predominantly 2D array was then
photographed from convergent camera positions to
simulate a 3D array, resulting in the geometrically strong
network detailed in figure 1. To strengthen further the
network and enable a more precise recovery of camera
inner orientation parameters, additional photographs were
taken with cameras rotated by 90 degrees about their
optical axis.