brightness value will again be affected.
Three methods of resampling are commonly used. The
first, the nearest neighbour method, takes the
value of the pixel in the input image that is
closest to the newly-computed centres. The second,
bilinear interpolation, takes the average of the
four pixels nearest to the new coordinates. The
third method, cubic convolution, computes the new
pixel value taking into account the 16 nearest
pixels in the input image.
A more complete description of the traditional
techniques for geometric rectification as well for
resampling can be found in Jensen (1986) and Mather
(1987).
2.3 Application of Traditional Techniques
A geometric rectification was carried out on the
ATM image of Antequera using the least squares
polynomial fit method described in section 2.2. It
was based on the selection of 71 ground control
points reasonably well distributed in the image.
The UTM geographic coordinates of the points were
taken from the 1:10 000 topographic maps and the
image coordinates from a display of the image on
the Nottingham Image Processing System, NIPS.
The results from the first order polynomial
transformation showed some large residuals, of the
order of 13 pixels, for both column and row. The
Root Mean Square Error (RMSE) for columns was 5.8
and for rows was 5.7 pixels. The results from the
second order polynomial showed only a small
improvement with RMSE values of 5.6 and 4.5 pixels
for column and row respectively. A substantial
improvement was achieved with the third order
polynomial with the majority of residuals being
within £4 pixels with RMSE values of 2.5 and 1.8
for column and row respectively.
A visual assessment of the effects of the
transformations on the image was obtained by
producing a corrected image for each order of
polynomial and then overlaying the digitized map.
The overlay was accomplished by clipping each
corrected image by a number of rows and columns in
order to get the best match with the map centre.
As might be expected, the visual inspection showed
increasing displacements of the corresponding
features in the two images from the centre to the
edges. The displacements were, as expected, bigger
in the first and second order corrected images and
smaller for the third order corrected image. The
third order corrected image showed larger residuals
than were acceptable.
2.4 Geometric Characteristics of the Image
The basic geometric operation of the ATM is given
in section 3.2.
In addition to the instrumental characteristics
that affect the geometry of the image there are a
number of external influences. These fall into two
groups: those that are inherent in the geometry of
the system and those that are due to operational
difficulties and problems.
The velocity to height ratio (V/H), the scan rate
of the scanning mirror and the ground resolution,
as well as the swath width are defined by the
flying height above the ground level. Incorrect
adjustment of the scanning mirror speed will cause
under or over scanning and thus influence the
geometry. There will also be a change in the
ground resolution element size with different scan
angles (see section 3.2). A variation in the
ground relief will result in image displacement,
which is a similar problem to that experienced in
conventional aerial photography.
has
The sensor platform, being aircraft-based,
16
significant inherent instabilities, due to the
characteristics of the aircraft motion and the
atmospheric conditions in which it operates. To
assist with minimising the effects of aircraft
roll, up to a maximum of #15 degrees, a gyro
assembly monitors the aircraft and only allows the
image to be collected within an angle of
approximately 37 degrees either side of the
vertical.
As mentioned above, for the polynomial technique to
be fully effective dt not only "performs à
transformation but corrects for the systematic
errors present. It is extremely difficult to model
the effect on the image geometry of all the above
mentioned influences. Therefore, a more direct
modelling technique could be employed.
3. TIME-DEPENDENT GEOMETRY METHOD FOR
RECTIFICATION OF IMAGES
3.1 Introduction
The basic principle of the technique discussed so
far is that of modelling systematic errors in the
image. The model is defined by a polynomial which
should describe the systematic errors present. The
polynomial should be based on an analysis of the
influences affecting the geometry of the imaging
system. Therefore the choice of polynomial is
important to obtain the optimum results. An
alternative approach to solving the problem is to
attempt to model the cause rather than, as in the
polynomial case, the effects on the image. The use
of the collinearity equations in digital image
processing is not new (Konecny, 1979), also the use
of time-dependent geometry is not a new concept (El
Hassin, 1981; Smith, 1989) although it is becoming
more popular with developments in analytical and
digital techniques. For this reason the solution
presented here attempts to remain as general, for
any similar sensor, as possible. The geometry of
the imaging system must be analysed and modelled,
which, in the case being considered here, involves
the sensor geometry and the aircraft motion during
the period of imaging. The principles of the
sensor geometry are reasonably well documented
where as the aircraft motion is not accurately
known and requires certain assumptions to be made.
3.2 Analysis of the Imaging System Geometry
The sensing system consists of a rotating mirror
that scans a swath of ground to either side of
nadir. A scan line of data is collected as à
series of 2.5 mrad instantaneous fields of view
(IF0V), which therefore defines the resolution.
Since the image data is captured in relation to a
constant angular measure and constant pixel unit
size, the ground area covered by the IFOV will vary
depending on the angle from nadir, resulting in
compression of the image towards the edges. This
is removed from the image by the S-bend correction
in the digitization process. So the fundamental
Scanning geometry being described is therefore
perspective geometry if the sensor was stationary.
Successive scan lines of adjoining ground swath are
produced by the forward motion of the aircraft.
The butting together of the scan lines is dependent
largely on the velocity-to-height ratio of the
aircraft, although this is controlled by the
allowable scan rates and the required resolution
(as mentioned above). Normally these are selected
to ensure some overlap, typically 10%. So the
aircraft motion has an effect on the scan geometry
(perspective geometry) and is used to create the
series of scan lines to produce the image. It is
therefore necessary to attempt to describe the
aircraft motion during the image capture.
Considering the rate at which the image is
captured, scan rates available are 12.5, 25 or 50
scans/sec, for an image of 1000 scan lines (the
approximate image size being considered), the time
to capture the image would be 80, 40 or 20 seconds